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Results 1 - 58 of 58
The R-Process Alliance: Analysis of Limited-r Stars
Volume 19, Issue 14 - article #4
T. Xylakis-Dornbusch
,
T. T. Hansen
,
T. C. Beers
,
N. Christlieb
,
R. Ezzeddine
,
A. Frebel
,
E. Holmbeck
,
V. M. Placco
,
I. U. Roederer
,
C. M. Sakari
,
C. Sneden
https://arxiv.org/abs/2404.03379
Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk. (arXiv:2308.01928v1 [astro-ph.GA])
Volume 18, Issue 32 - article #5
R. da Silva
,
V. D'Orazi
,
M. Palla
,
G. Bono
,
V.F. Braga
,
M. Fabrizio
,
B. Lemasle
,
E. Spitoni
,
F. Matteucci
,
H. Jonsson
,
V. Kovtyukh
,
L. Magrini
,
M. Bergemann
,
M. Dall'Ora
,
I. Ferraro
,
G. Fiorentino
,
P. Francois
,
G. Iannicola
,
L. Inno
,
R.-P. Kudritzki
,
N. Matsunaga
,
M. Monelli
,
M. Nonino
,
C. Sneden
,
J. Storm
,
F. Thevenin
,
T. Tsujimoto
,
A. Zocchi
http://arxiv.org/abs/2308.01928
Chemical Evolution of Ytterbium in the Galactic Disk. (arXiv:2202.00691v1 [astro-ph.GA])
Volume 17, Issue 5 - article #3
M. Montelius
,
R. Forsberg
,
N. Ryde
,
H. Jönsson
,
M. Afşar
,
A. Johanssen
,
K. F. Kaplan
,
H. Kim
,
G. Mace
,
C. Sneden
,
B. Thorsbro
http://arxiv.org/abs/2202.00691
On the Use of Field RR Lyrae as Galactic Probes. V. Optical and Radial Velocity Curve Templates
Volume 16, Issue 40 - article #6
V. F. Braga
,
J. Crestani
,
M. Fabrizio
,
G. Bono
,
C. Sneden
,
G. W. Preston
,
J. Storm
,
S. Kamann
,
M. Latour
,
H. Lala
,
B. Lemasle
,
Z. Prudil
,
G. Altavilla
,
B. Chaboyer
,
M. Dall’Ora
,
I. Ferraro
,
C. K. Gilligan
,
G. Fiorentino
,
G. Iannicola
,
L. Inno
,
S. Kwak
,
M. Marengo
,
S. Marinoni
,
P. M. Marrese
,
C. E. MartÃÂnez-Vázquez
,
M. Monelli
,
J. P. Mullen
,
N. Matsunaga
,
J. Neeley
,
P. B. Stetson
,
E. Valenti,
,
M. Zoccali
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/919/2/85
On the Use of Field RR Lyrae As Galactic Probes: IV. New Insights Into and Around the Oosterhoff Dichotomy
Volume 16, Issue 40 - article #7
M. Fabrizio
,
V. F. Braga
,
J. Crestani
,
G. Bono
,
I. Ferraro
,
G. Fiorentino
,
G. Iannicola
,
G. W. Preston
,
C. Sneden
,
F. Thévenin
,
G. Altavilla
,
B. Chaboyer
,
M. Dall’Ora
,
R. da Silva
,
E. K. Grebel
,
C. K. Gilligan
,
H. Lala
,
B. Lemasle
,
D. Magurno
,
M. Marengo
,
S. Marinoni
,
P. M. Marrese
,
C. E. MartÃÂnez-Vázquez
,
N. Matsunaga
,
M. Monelli
,
J. P. Mullen
,
J. Neeley
,
M. Nonino
,
Z. Prudil
,
M Salaris
,
P. B. Stetson
,
E. Valenti,
,
M. Zoccali
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/919/2/118
Heavy elements in barium stars. (arXiv:2108.08132v1 [astro-ph.SR])
Volume 16, Issue 34 - article #1
M. P. Roriz
,
M. Lugaro
,
C. B. Pereira
,
C. Sneden
,
S. Junqueira
,
A. I. Karakas
,
N. A. Drake
http://arxiv.org/abs/2108.08132
On the Use of Field RR Lyrae as Galactic Probes. III. The $alpha$-element abundances. (arXiv:2104.08113v1 [astro-ph.GA])
Volume 16, Issue 17 - article #2
J. Crestani
(1,2,3),
V.F. Braga
(3,4),
M. Fabrizio
(3,4),
G. Bono
(2,3),
C. Sneden
(5),
G.W. Preston
(6),
I. Ferraro
(3),
G. Iannicola
(3),
M. Nonino
(7),
G. Fiorentino
(3),
F. Thévenin
(8),
B. Lemasle
(9),
Z. Prudil
(8),
A. Alves-Brito
(1),
G. Altavilla
(3,4),
B. Chaboyer
(10),
M. Dall'Ora
(11),
V. D'Orazi
(12,13),
C.K. Gilligan
(10),
E. Grebel
(8),
A.J. Koch-Hansen
(9),
H. Lala
(9),
M. Marengo
(14),
S. Marinoni
(3,4),
P.M. Marrese
(3,4),
C.E. Martínez-Vázquez
(15),
N. Matsunaga
(16),
M. Monelli
(17),
J.P. Mullen
(14),
J. Neeley
(18),
R. da Silva
(3,4),
P.B. Stetson
(19),
M. Salaris
(20),
J. Storm
(21),
E. Valenti
(22),
M. Zoccali
(23,24)
((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(4) Space Science Data Center, Roma, Italy,
(5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy,
(8) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(9) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany,
(10) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(11) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(12) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(13) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia,
(14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(15) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(16) Department of Astronomy, The University of Tokyo, Tokyo, Japan,
(17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(18) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(19) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada,
(20) Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK,
(21) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany,
(22) European Southern Observatory, Garching bei Munchen, Germany,
(23) Instituto Milenio de Astrofísica, Santiago, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/2104.08113
On the Use of Field RR Lyrae as Galactic Probes. II. A new $Delta$S calibration to estimate their metallicity. (arXiv:2012.02284v1 [astro-ph.SR])
Volume 15, Issue 50 - article #6
J. Crestani
(1,2,3),
M. Fabrizio
(3,4),
V.F. Braga
(3,4),
C. Sneden
(5),
G.W. Preston
(6),
I. Ferraro
(3),
G. Iannicola
(3),
G. Bono
(2,3),
A. Alves-Brito
(1),
M. Nonino
(7),
V. D'Orazi
(8,9),
L. Inno
(10),
M. Monelli
(11),
J. Storm
(12),
G. Altavilla
(3,4),
B. Chaboyer
(13),
M. Dall'Ora
(14),
G. Fiorentino
(3),
C.K. Gilligan
(13),
E. Grebel
(15),
H. Lala
(16),
B. Lemasle
(16),
M. Marengo
(17),
S. Marinoni
(3,4),
P.M. Marrese
(3,4),
C.E. Martínez-Vázquez
(18),
N. Matsunaga
(19),
J.P. Mullen
(17),
J. Neeley
(20),
Z. Prudil
(15),
R. da Silva
(3,4),
P.B. Stetson
(21),
F. Thévenin
(15),
E. Valenti
(22),
A.R. Walker
(18),
M. Zoccali
(23,24)
((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(4) Space Science Data Center, Roma, Italy,
(5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy,
(8) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(9) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia,
(10) Università degli Studi di Napoli "Parthenope'', Napoli, Italy,
(11) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(12) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany,
(13) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(14) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(15) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(16) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany,
(17) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(18) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(19) Department of Astronomy, The University of Tokyo, Tokyo, Japan,
(20) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(21) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada,
(22) European Southern Observatory, Garching bei Munchen, Germany,
(23) Instituto Milenio de Astrofísica, Santiago, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/2012.02284
A Chemo-dynamical Link between the Gjöll Stream and NGC 3201
Volume 15, Issue 38 - article #9
T. T. Hansen
,
A. H. Riley
,
L. E. Strigari
,
J. L. Marshall
,
P. S. Ferguson
,
J. Zepeda,
,
C. Sneden
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/901/1/23
A chemo-dynamical link between the Gj"oll stream and NGC 3201. (arXiv:2007.12165v1 [astro-ph.SR])
Volume 15, Issue 30 - article #2
T. T. Hansen
,
A. H. Riley
,
L. E. Strigari
,
J. L. Marshall
,
P. S. Ferguson
,
J. Zepeda
,
C. Sneden
http://arxiv.org/abs/2007.12165
On the Metamorphosis of the Bailey Diagram for RR Lyrae Stars
Volume 15, Issue 24 - article #28
G. Bono
,
V. F. Braga
,
J. Crestani
,
M. Fabrizio
,
C. Sneden
,
M. Marconi
,
G. W. Preston
,
J. P. Mullen
,
C. K. Gilligan
,
G. Fiorentino
,
A. Pietrinferni
,
G. Altavilla
,
R. Buonanno
,
B. Chaboyer
,
R. da Silva
,
M. Dall’Ora
,
S. Degl’Innocenti
,
E. Di Carlo
,
I. Ferraro
,
E. K. Grebel
,
G. Iannicola
,
L. Inno
,
V. Kovtyukh
,
A. Kunder
,
B. Lemasle
,
M. Marengo
,
S. Marinoni
,
P. M. Marrese
,
C. E. MartÃÂnez-Vázquez
,
N. Matsunaga
,
M. Monelli
,
J. Neeley
,
M. Nonino
,
P. G. Prada Moroni
,
Z. Prudil
,
P. B. Stetson
,
F. Thévenin
,
E. Tognelli
,
E. Valenti,
,
A. R. Walker
The Astrophysical Journal Letters
http://iopscience.iop.org/2041-8205/896/1/L15
On the Use of Field RR Lyrae as Galactic Probes. I. The Oosterhoff Dichotomy Based on Fundamental Variables
Volume 14, Issue 38 - article #16
M. Fabrizio
,
G. Bono
,
V. F. Braga
,
D. Magurno
,
S. Marinoni
,
P. M. Marrese
,
I. Ferraro
,
G. Fiorentino
,
G. Giuffrida
,
G. Iannicola
,
M. Monelli
,
G. Altavilla
,
B. Chaboyer
,
M. Dall’Ora
,
C. K. Gilligan
,
A. Layden
,
M. Marengo
,
M. Nonino
,
G. W. Preston
,
B. Sesar
,
C. Sneden
,
E. Valenti
,
F. Thévenin,
,
E. Zoccali
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/882/2/169
Chemical Compositions of Field and Globular Cluster RR Lyrae Stars. II. ω Centauri
Volume 14, Issue 34 - article #10
D. Magurno
,
C. Sneden
,
G. Bono
,
V. F. Braga
,
M. Mateo
,
S. E. Persson
,
G. Preston
,
F. Thévenin
,
R. da Silva
,
M. Dall’Ora
,
M. Fabrizio
,
I. Ferraro
,
G. Fiorentino
,
G. Iannicola
,
L. Inno
,
M. Marengo
,
S. Marinoni
,
P. M. Marrese
,
C. E. MartÃÂnez-Vázquez
,
N. Matsunaga
,
M. Monelli
,
J. R. Neeley
,
M. Nonino,
,
A. R. Walker
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/881/2/104
Chemical Compositions of Field and Globular Cluster RR~Lyrae Stars: II. omega Centauri. (arXiv:1906.08550v1 [astro-ph.SR])
Volume 14, Issue 25 - article #2
D. Magurno
(1, 2, 3),
C. Sneden
(4),
G. Bono
(1, 2),
V. F. Braga
(5, 6),
M. Mateo
(7),
S. E. Persson
(8),
G. Preston
(8),
F. Thevenin
(9),
R. da Silva
(10),
M. Dall'Ora
(11),
M. Fabrizio
(2, 10),
I. Ferraro
(2),
G. Fiorentino
(12),
G. Iannicola
(2),
L. Inno
(13),
M. Marengo
(14),
S. Marinoni
(10),
P. M. Marrese
(10),
C. E. Martinez-Vazquez
(15),
N. Matsunaga
(16),
M. Monelli
(17),
J. R. Neeley
(18),
M. Nonino
(19),
A. R. Walker
(15)
((1) University of Roma Tor Vergata - Department of Physics - Roma - Italy,
(2) INAF Osservatorio Astronomico di Roma - Monte Porzio Catone RM - Italy,
(3) University of Bologna - Department of Physics, Astronomy - Bologna - Italy,
(4) Department of Astronomy, McDonald Observatory - The University of Texas - Austin - TX - USA,
(5) Instituto Milenio de Astrofisica - Santiago - Chile,
(6) Departamento de Fisica - Facultad de Ciencias Exactas - Universidad Andres Bello - Las Condes - Santiago - Chile,
(7) Department of Astronomy - University of Michigan - Ann Arbor - MI - USA,
(8) Observatories of the Carnegie Institution for Science - Pasadena - CA 91101 - USA,
(9) Universite de La Cote d'Azur - OCA - Laboratoire Lagrange CNRS - Nice Cedex - France,
(10) SSDC - via del Politecnico snc - I-00133 Roma - Italy,
(11) INAF Osservatorio Astronomico di Capodimonte - Salita Moiariello 16 - Napoli - Italy,
(12) INAF Osservatorio Astronomico di Bologna - Via Ranzani 1 - Bologna - Italy,
(13) Max Planck Institute fur Astronomie - Konigstuhl - Heidelberg - Germany,
(14) Department of Physics, Astronomy - Iowa State University - Zaffarano - Ames - IA - USA,
(15) Cerro Tololo Inter-American Observatory - National Optical Astronomy Observatory - Casilla - La Serena - Chile,
(16) Department of Astronomy - The University of Tokyo - Hongo - Bunkyo-ku - Tokyo - Japan,
(17) IAC - Instituto de Astrofsica de Canarias - Calle Via Lactea - La Laguna - Tenerife - Espana,
(18) Department of Physics - Florida Atlantic University - Boca Raton - FL - USA,
(19) INAF Osservatorio Astronomico di Trieste - Trieste - Italy)
http://arxiv.org/abs/1906.08550
On a New Method to Estimate the Distance, Reddening, and Metallicity of RR Lyrae Stars Using Optical/Near-infrared ( B, V, I, J, H, K ) Mean Magnitudes: ω Centauri as a First Test Case
Volume 14, Issue 3 - article #14
G. Bono
,
G. Iannicola
,
V. F. Braga
,
I. Ferraro
,
P. B. Stetson
,
D. Magurno
,
N. Matsunaga
,
R. L. Beaton
,
R. Buonanno
,
B. Chaboyer
,
M. Dall’Ora
,
M. Fabrizio
,
G. Fiorentino
,
W. L. Freedman
,
C. K. Gilligan
,
B. F. Madore
,
M. Marconi
,
M. Marengo
,
S. Marinoni
,
P. M. Marrese
,
C. E. Martinez-Vazquez
,
M. Mateo
,
M. Monelli
,
J. R. Neeley
,
M. Nonino
,
C. Sneden
,
F. Thevenin
,
E. Valenti,
,
A. R. Walker
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/870/2/115
On a new method to estimate distance, reddening and metallicity of RR Lyrae stars using optical/near-infrared ($B$,$V$,$I$,$J$,$H$,$K$) mean magnitudes: $omega$ Centauri as a first test case. (arXiv:1811.07069v1 [astro-ph.SR])
Volume 13, Issue 47 - article #2
G. Bono
(1, 2),
G. Iannicola
(2),
V.F. Braga
(3, 4),
I. Ferraro
(2),
P.B. Stetson
(5),
D. Magurno
(1),
N. Matsunaga
(6),
R.L. Beaton
(7),
R. Buonanno
(8),
B. Chaboyer
(9),
M. Dall'Ora
(10),
M. Fabrizio
(2, 11),
G. Fiorentino
(12),
W.L. Freedman
(13,7),
C.K. Gilligan
(9),
B.F. Madore
(7),
M. Marconi
(10),
M. Marengo
(14),
S. Marinoni
(2, 11),
P. Marrese
(2, 11),
C.E. Martinez-Vazquez
(15),
M. Mateo
(16),
M. Monelli
(17, 18),
J.R. Neeley
(19),
M. Nonino
(20),
C. Sneden
(21),
F. Thevenin
(22),
E. Valenti
(23),
A.R. Walker
(15)
((1) Department of Physics, Università di Roma Tor Vergata, Roma, Italy,
(2) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(3) Instituto Milenio de Astrofisica, Santiago, Chile,
(4) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile,
(5) NRC-Herzberg, Dominion Astrophysical Observatory, Victoria BC, Canada,
(6) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Nagano Japan,
(7) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(8) INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy,
(9) Department of Physics, Astronomy, Dartmouth College, Hanover, NH, USA,
(10) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(11) SSDC, Roma, Italy,
(12) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy,
(13) Department of Astronomy, Astrophysics, University of Chicago, Chicago, IL, USA,
(14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(15) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile,
(16) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA,
(17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(18) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain,
(19) Department of Physics, Florida Atlantic University, Boca Raton, FL 33431, USA,
(20) INAF-Osservatorio Astronomico di Trieste, Trieste, Italy,
(21) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(22) Universite de Nice Sophia-antipolis, CNRS, Observatoire de la Cote d'Azur, Laboratoire Lagrange, Nice, France,
(23) European Southern Observatory, Garching bei Munchen, Germany)
http://arxiv.org/abs/1811.07069
Transition Probabilities of Co ii Weak Lines to the Ground and Low Metastable Levels
Volume 13, Issue 36 - article #19
J. E. Lawler
,
T. Feigenson
,
C. Sneden
,
J. J. Cowan,
,
G. Nave
The Astrophysical Journal Supplement Series
http://iopscience.iop.org/0067-0049/238/1/7
Chemical Compositions of Field and Globular Cluster RR Lyrae Stars. I. NGC 3201
Volume 13, Issue 35 - article #13
D. Magurno
,
C. Sneden
,
V. F. Braga
,
G. Bono
,
M. Mateo
,
S. E. Persson
,
M. Dall’Ora
,
M. Marengo
,
M. Monelli,
,
J. R. Neeley
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/864/1/57
Chemical Compositions of Field and Globular Cluster RR Lyrae Stars: I. NGC 3201. (arXiv:1807.06681v1 [astro-ph.SR])
Volume 13, Issue 29 - article #3
D. Magurno
,
C. Sneden
,
V. F. Braga
,
G. Bono
,
M. Mateo
,
S. E. Persson
,
M. Dall'Ora
,
M. Marengo
,
M. Monelli
,
J. R. Neeley
http://arxiv.org/abs/1807.06681
Impact of distance determinations on Galactic structure. II. Old tracers. (arXiv:1806.07487v1 [astro-ph.GA])
Volume 13, Issue 25 - article #3
A. Kunder
,
E. Valenti
,
M. Dall'Ora
,
P. Pietrukowicz
,
C. Sneden
,
G. Bono
,
V.F. Braga
,
I. Ferraro
,
G. Fiorentino
,
G. Iannicola
,
M. Marconi
,
C. E. Martinez-Vazquez
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M. Monelli
,
I. Musella
,
V. Ripepi
,
M. Salaris
,
P.B. Stetson
http://arxiv.org/abs/1806.07487
Improved Cr II log(gf) Values and Abundance Determinations in the Photospheres of the Sun and Metal-poor Star HD 84937
Volume 12, Issue 4 - article #14
J. E. Lawler
,
C. Sneden
,
G. Nave
,
E. A. Den Hartog
,
N. Emrahoğlu,
,
J. J. Cowan
The Astrophysical Journal Supplement Series
http://iopscience.iop.org/0067-0049/228/1/10
Discovery of a Metal-poor Field Giant with a Globular Cluster Second-generation Abundance Pattern
Volume 11, Issue 51 - article #14
J. G. Fernández-Trincado
,
A. C. Robin
,
E. Moreno
,
R. P. Schiavon
,
A. E. GarcÃÂa Pérez
,
K. Vieira
,
K. Cunha
,
O. Zamora
,
C. Sneden
,
Diogo Souto
,
R. Carrera
,
J. A. Johnson
,
M. Shetrone
,
G. Zasowski
,
D. A. GarcÃÂa-Hernández
,
S. R. Majewski
,
C. Reylé
,
S. Blanco-Cuaresma
,
L. A. Martinez-Medina
,
A. Pérez-Villegas
,
O. Valenzuela
,
B. Pichardo
,
A. Meza
,
Sz. Mészáros
,
J. Sobeck
,
D. Geisler
,
F. Anders
,
M. Schultheis
,
B. Tang
,
A. Roman-Lopes
,
R. E. Mennickent
,
K. Pan
,
C. Nitschelm,
,
F. Allard
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/833/2/132
Discovery of a Metal-Poor Field Giant with a Globular Cluster Second-Generation Abundance Pattern. (arXiv:1604.01279v2 [astro-ph.GA] UPDATED)
Volume 11, Issue 41 - article #2
J. G. Fernández-Trincado
,
A. C. Robin
,
E. Moreno
,
R. P. Schiavon
,
A. E. García Peréz
,
K. Vieira
,
K. Cunha
,
O. Zamora
,
C. Sneden
,
Diogo Souto
,
R. Carrera
,
J. A. Johnson
,
M. Shetrone
,
G. Zasowski
,
D. A. García-Hernández
,
S. R. Majewski
,
C. Reylé
,
S. Blanco-Cuaresma
,
L. A. Martinez-Medina
,
A. Pérez-Villegas
,
O. Valenzuela
,
B. Pichardo
,
A. Meza
,
Sz. Mészáros
,
J. Sobeck
,
D. Geisler
,
F. Anders
,
M. Schultheis
,
B. Tang
,
A. Roman-Lopes
,
R. E. Mennickent
,
K. Pan
,
C. Nitschelm
,
F. Allard
http://arxiv.org/abs/1604.01279
Discovery of a Metal-Poor Field Giant with a Globular Cluster Second-Generation Abundance Pattern
Volume 11, Issue 15 - article #1
J. G. Fernandez-Trincado
,
A. C. Robin
,
E. Moreno
,
R. P. Schiavon
,
A. E. García Peréz
,
K. Vieira
,
K. Cunha
,
O. Zamora
,
C. Sneden
,
R. Carrera
,
J. A. Johnson
,
M. Shetrone
,
G. Zasowski
,
D. A. García-Hernándes
,
S. R. Majewski
,
C. Reylé
,
S. Blanco-Cuaresma
,
L. A. Martinez-Medina
,
A. Pérez-Villegas
,
O. Valenzuela
,
B. Pichardo
,
A. Meza
,
Sz. Mészáros
,
J. Sobeck
,
D. Geisler
,
F. Anders
,
M. Schultheis
,
B. Tang
,
A. Roman-Lopes
,
R. E. Mennickent
,
K. Pan
,
C. Nitschelm
,
F. Allard
arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Apr
arXiv:1604.01279
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The MÂ 4 Core Project with
HST
– IV. Internal kinematics from accurate radial velocities of 2771 cluster members
Volume 10, Issue 41 - article #16
L. Malavolta
,
G. Piotto
,
L. R. Bedin
,
C. Sneden
,
V. Nascimbeni
,
and
V. Sommariva
Monthly Notices of the Royal Astronomical Society - Volume: 454, Issue: 3
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Volume 10, Issue 34 - article #9
L. Malavolta
,
G. Piotto
,
L. R. Bedin
,
C. Sneden
,
V. Nascimbeni
,
V. Sommariva
arXiv.org - Astrophysics - Volume: 2015, Issue: 18 Sep
arXiv:1509.05048
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A Detailed Study of Giants and Horizontal Branch Stars in M68: Atmospheric Parameters and Chemical Abundances
Volume 10, Issue 21 - article #15
M. Schaeuble
,
G. Preston
,
C. Sneden
,
I. B. Thompson
,
S. A. Shectman
,
and
G. S. Burley
Astronomical Journal - Volume: 149, Issue: 6
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The Chemical Compositions and Evolutionary Status of Red Giants in the Open Cluster NGC 752
Volume 9, Issue 25 - article #32
G. Böcek Topcu
,
M. Afşar
,
M. Schaeuble
,
C. Sneden
arXiv.org - Astrophysics - Volume: 2014, Issue: 5 Dec
arXiv:1411.7608
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The chemical compositions and evolutionary status of red giants in the open cluster NGC 752
Volume 9, Issue 25 - article #51
G. Böcek Topcu
,
M. Afşar
,
M. Schaeuble
,
and
C. Sneden
Monthly Notices of the Royal Astronomical Society - Volume: 446, Issue: 4
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Searching for Chemical Signatures of Multiple Stellar Populations in the Old, Massive Open Cluster NGC 6791
Volume 9, Issue 23 - article #30
A. Bragaglia
(1),
C. Sneden
(2,3,4),
E. Carretta
(1),
R.G. Gratton
(4),
S. Lucatello
(4),
P.F. Bernath
(5),
J.S.A. Brooke
(6),
R.S. Ram
(6)
(1-INAF OA Bologna, 2-Dept. Astronomy & McDonals Obs. Austin, TX, 3-Ege Univ. Izmir, 4-INAF OA Padova, 5-Old Dominion Univ. Norfolk, VA, 6-Univ. of York)
arXiv.org - Astrophysics - Volume: 2014, Issue: 3 Oct
arXiv:1409.8283
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Improved Ni I log(gf) Values and Abundance Determinations in the Photospheres of the Sun and Metal-poor Star HD 84937
Volume 9, Issue 8 - article #2
M. P. Wood
,
J. E. Lawler
,
C. Sneden
,
J. J. Cowan
arXiv.org - Astrophysics - Volume: 2014, Issue: 21 Feb
arXiv:1402.4457
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Improved Log(
gf
) Values for Lines of Ti I and Abundance Determinations in the Photospheres of the Sun and Metal-Poor Star HD 84937 (Accurate Transition Probabilities for Ti I)
Volume 8, Issue 50 - article #27
J. E. Lawler
,
A. Guzman
,
M. P. Wood
,
C. Sneden
,
and
J. J. Cowan
The Astrophysical Journal Supplement - Volume: 205, Issue: 2
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Potassium in Globular Cluster Stars: Comparing Normal Clusters to the Peculiar Cluster NGCÂ 2419
Volume 8, Issue 20 - article #21
E. Carretta
,
R. G. Gratton
,
A. Bragaglia
,
V. D'Orazi
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S. Lucatello
,
A. Sollima
,
and
C. Sneden
The Astrophysical Journal - Volume: 769, Issue: 1
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First stars - XVI. HST/STIS abundances of heavy elements in the uranium-rich metal-poor star CS 31082-001
Volume 8, Issue 7 - article #21
C. Siqueira Mello Jr.
,
M. Spite
,
B. Barbuy
,
F. Spite
,
E. Caffau
,
V. Hill
,
S. Wanajo
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F. Primas
,
B. Plez
,
R. Cayrel
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et al.
(7 more)J.
Andersen
,
B. Nordström
,
C. Sneden
,
T. C. Beers
,
P. Bonifacio
,
P. François
and
P. Molaro
Astronomy and Astrophysics - Volume: 550, Issue: February 2013
http://dx.doi.org/10.1051/0004-6361/201219949
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Chemical Compositions of Thin-disk, High-metallicity Red Horizontal-branch Field Stars
Volume 7, Issue 51 - article #15
M. Afşar
,
C. Sneden
,
and
B.-Q. For
Astronomical Journal - Volume: 144, Issue: 1
doi:10.1088/0004-6256/144/1/20
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Searching for multiple stellar populations in the massive, old open cluster Berkeley 39
Volume 7, Issue 51 - article #86
A. Bragaglia
,
R. G. Gratton
,
E. Carretta
,
V. D’Orazi
,
C. Sneden
and
S. Lucatello
Astronomy and Astrophysics - Volume: 548, Issue: December 2012
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First stars XVI. STIS/HST abundances of heavy-elements in the uranium-rich star CS 31082-001
Volume 7, Issue 49 - article #6
C. Siqueira Mello
,
M. Spite
,
B. Barbuy
,
F. Spite
,
E. Caffau
,
V. Hill
,
S. Wanajo
,
F. Primas
,
B. Plez
,
R. Cayrel
,
J. Andersen
,
B. Nordström
,
C. Sneden
,
T. C. Beers
,
P. Bonifacio
,
P. François
,
P. Molaro
arXiv.org - Astrophysics - Volume: 2012, Issue: 7 Dec
arXiv:1212.0211
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Searching for multiple stellar populations in the massive, old open cluster Berkeley 39
Volume 7, Issue 45 - article #9
A. Bragaglia
(1),
R.G. Gratton
(2),
E. Carretta
(1),
V. D'Orazi
(3,4),
C. Sneden
(5),
S. Lucatello
(2)
(1-INAF OA Bologna, 2-INAF OA Padova, 3- Macquarie Univ., 4-Monash Univ., 5-Univ. of Texas Austin)
arXiv.org - Astrophysics - Volume: 2012, Issue: 9 Nov
arXiv:1211.1142
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Chemical compositions of thin-disk, high-metallicity red horizontal-branch field stars
Volume 7, Issue 20 - article #5
M. Afşar
,
C. Sneden
,
B.-Q. For
arXiv.org - Astrophysics - Volume: 2012, Issue: 18 May
arXiv:1205.3659
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The double sub-giant branch of NGC 6656 (M22): a chemical characterization
Volume 7, Issue 7 - article #16
A. F. Marino
,
A. P. Milone
,
C. Sneden
,
M. Bergemann
,
R. P. Kraft
,
G. Wallerstein
,
S. Cassisi
,
A. Aparicio
,
M. Asplund
,
R. L. Bedin
,
M. Hilker
,
K. Lind
,
Y. Momany
,
G. Piotto
,
I. U. Roederer
,
P. B. Stetson
,
M. Zoccali
arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Feb
arXiv:1202.2825
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Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups
Volume 6, Issue 47 - article #21
I. U. Roederer
,
A. F. Marino
and
C. Sneden
The Astrophysical Journal - Volume: 742, Issue: 1
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Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups
Volume 6, Issue 34 - article #6
I.U. Roederer
,
A.F. Marino
,
C. Sneden
arXiv.org - Astrophysics - Volume: 2011, Issue: 26 Aug
arXiv:1108.3868
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Chemically tagging the Hyades stream: does it partly originate from the Hyades cluster?
Volume 6, Issue 29 - article #23
L. Pompéia
,
T. Masseron
,
B. Famaey
,
S. Van Eck
,
A. Jorissen
,
I. Minchev
,
A. Siebert
,
C. Sneden
,
J. R. D. Lépine
,
C. Siopis
,
G. Gentile
,
T. Dermine
,
E. Pasquato
,
H. Van Winckel
,
C. Waelkens
,
G. Raskin
,
S. Prins
,
W. Pessemier
,
H. Hensberge
,
Y. Frémat
,
L. Dumortier
and
O. Bienaymé
,
Monthly Notices of the Royal Astronomical Society - Volume: 415, Issue: 2
Abstract
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The two metallicity groups of the globular cluster M22: a chemical perspective
Volume 6, Issue 19 - article #18
A. F. Marino
,
C. Sneden
,
R. P. Kraft
,
G. Wallerstein
,
J. E. Norris
,
G. Da Costa
,
A. P. Milone
,
I. I. Ivans
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G. Gonzalez
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J. P. Fulbright
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M. Hilker
,
G. Piotto
,
M. Zoccali
,
P. B. Stetson
arXiv.org - Astrophysics - Volume: 2011, Issue: 13 May
arXiv:1105.1523
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The Abundances of Neutron Capture Species in the Very Metal-Poor Globular Cluster M15: An Uniform Analysis of RGB and RHB Stars
Volume 6, Issue 10 - article #18
J. S. Sobeck
,
R. P. Kraft
,
C. Sneden
,
G. W. Preston
,
J. J. Cowan
,
G. H. Smith
,
I. B. Thompson
,
S. A. Shectman
,
G. S. Burley
arXiv.org - Astrophysics - Volume: 2011, Issue: 11 Mar
arXiv:1103.1008
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Chemically tagging the Hyades stream: Does it partly originate from the Hyades cluster?
Volume 6, Issue 2 - article #3
L. Pompéia
,
T. Masseron
,
B. Famaey
,
S. Van Eck
,
A. Jorissen
,
I. Minchev
,
A. Siebert
,
C. Sneden
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J.R.D. Lépine
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C. Siopis
,
G. Gentile
,
T. Dermine
,
E. Pasquato
,
H. Van Winckel
,
C. Waelkens
,
G. Raskin
,
S. Prins
,
W. Pessemier
,
H. Hensberge
,
Y. Frémat
,
L. Dumortier
,
O. Bienaymé
,
arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
arXiv:1101.2583
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The Ubiquity of the Rapid Neutron-Capture Process
Volume 5, Issue 39 - article #19
I.U. Roederer
,
J.J. Cowan
,
A.I. Karakas
,
K.-L. Kratz
,
M. Lugaro
,
J. Simmerer
,
K. Farouqi
,
C. Sneden
arXiv.org - Astrophysics - Volume: 2010, Issue: 24 Sep
arXiv:1009.4496
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X-shooter observations of main sequence stars in the globular cluster NGC 2808: first chemical tagging of a He-normal and a He-rich dwarf
Volume 5, Issue 31 - article #12
A. Bragaglia
(1),
E. Carretta
(1),
R.G. Gratton
(2),
S. Lucatello
(2),
A. Milone
(3),
G. Piotto
(3),
V. D'Orazi
(2),
S. Cassisi
(4),
C. Sneden
(5),
L.R. Bedin
(6)
((1) INAF-Oss. Astr. Bologna,
(2) INAF-Oss. Astr. Padova,
(3) Univ. Padova,
(4) INAF-Oss. Astr. Collurania,
(5) Dept. Astronomy and McDonald Obs.
(6) STScI)
arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
arXiv:1007.5299
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The case of the disappearing CN-strong AGB stars in Galactic globular clusters -- Preliminary Results
Volume 5, Issue 16 - article #9
S. W. Campbell
(1 and 2),
D. Yong
(3),
E. C. Wylie-de Boer
(3),
R. J. Stancliffe
(2),
J. C. Lattanzio
(2),
G. C. Angelou
(2),
F. Grundahl
(4),
C. Sneden
(5)
((1) Departament de Fisica i Enginyeria Nuclear, Universitat Politecnica de Catalunya, Barcelona, Spain,
(2) Centre for Stellar and Planetary Astrophysics, Monash University, Australia,
(3) Research School of Astronomy and Astrophysics, Australian National University, Australia,
(4) Department of Physics and Astronomy, Aarhus University, Denmark,
(5) Department of Astronomy and McDonald Observatory, University of Texas, Austin, USA)
arXiv.org - Astrophysics - Volume: 2010, Issue: 16 Apr
arXiv:1004.2249
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Improved Laboratory Transition Probabilities for Er ii and Application to the Erbium Abundances of the Sun and Five
r
-Process-rich, Metal-poor Stars
Volume 3, Issue 35 - article #20
J. E. Lawler
,
C. Sneden
,
J. J. Cowan
,
J.-F. Wyart
,
I. I. Ivans
,
J. S. Sobeck
,
M. H. Stockett
,
and
E. A. Den Hartog
The Astrophysical Journal Supplement - Volume: 178, Issue: 1
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Improved Laboratory Transition Probabilities for Er II and Applications to the Erbium Abundances of the Sun and Five r-Process Rich, Metal-Poor Stars
Volume 3, Issue 18 - article #6
J. E. Lawler
,
C. Sneden
,
J. J. Cowan
,
J.-F. Wyart
,
I. I. Ivans
,
J. S. Sobeck
,
M. H. Stockett
,
E. A. Den Hartog
arXiv.org - Astrophysics - Volume: 2008, Issue: 1 May
arXiv:0804.4465
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The SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution Spectroscopy of SDSS/SEGUE Field Stars
Volume 2, Issue 44 - article #47
C. Allende Prieto
(1),
T. Sivarani
(2),
T.C. Beers
(2),
Y.S. Lee
(2),
L. Koesterke
(1),
M. Shetrone
(1),
C. Sneden
(1),
D.L. Lambert
(1),
R. Wilhelm
(3),
C.M. Rockosi
(4),
D. Lai
(4),
B. Yanny
(5),
I.I. Ivans
(6),
J.A. Johnson
(7),
W. Aoki
(8),
C.A.L. Bailer-Jones
(9),
P. Re Fiorentin
(9)
((1) University of Texas,
(2) Michigan State University and JINA,
(3) Texas Tech University,
(4) U.C. Santa Cruz,
(5) FNAL,
(6) Carnegie Observatories and Princeton University,
(7) Ohio State University,
(8) National Astronomical Observatory of Japan,
(9) MPIA, Heidelberg)
arXiv.org - Astrophysics - Volume: 2007, Issue: 1 Nov
arXiv:0710.5780
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Improved Laboratory Transition Probabilities for Hf The Astrophysical Journal Supplement - Volume169, Issue 1II and Hafnium Abundances in the Sun and 10 Metal-poor Stars
Volume 2, Issue 9 - article #7
J. E. Lawler
,
E. A. Den Hartog
,
Z. E. Labby
,
C. Sneden
,
J. J. Cowan
,
and
I. I. Ivans
The Astrophysical Journal Supplement - Volume169, Issue 1
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FULL TEXT WITH ENHANCEMENTS
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r-Process Enhanced Halo Stars
Volume 1, Issue 38 - article #4
J. J. Cowan
,
C. Sneden
,
J. E. Lawler
,
E. A. Den Hartog
ArXiv - Astrophysics
astro-ph/0610412 [
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r-Process Enhanced Halo Stars
Volume 1, Issue 38 - article #4
J. J. Cowan
,
C. Sneden
,
J. E. Lawler
,
E. A. Den Hartog
ArXiv - Astrophysics
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Gd Transition Probabilities and Abundances
Volume 1, Issue 34 - article #6
E. A. Den Hartog
,
J. E. Lawler
,
C. Sneden
,
J. J. Cowan
ArXiv - Astrophysics
astro-ph/0609487 [
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Manganese Abundances in Cluster and Field Stars
Volume 1, Issue 15 - article #12
J.S. Sobeck
,
I.I. Ivans
,
J. A. Simmerer
,
C. Sneden
,
P. Hoeflich
,
J.P. Fulbright
,
R. P. Kraft
ArXiv - Astrophysics
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Improved Laboratory Transition Probabilities for Sm The Astrophysical Journal Supplement - Volume162, Issue 1II and Application to the Samarium Abundances of the Sun and Three
r
-Process–rich, Metal-poor Stars
Volume 1, Issue 1 - article #14
J. E. Lawler
,
E. A. Den Hartog
,
C. Sneden
,
and
J. J. Cowan
The Astrophysical Journal Supplement - Volume162, Issue 1
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