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Results 1 - 43 of 43
(Re)mind the gap: a hiatus in star formation history unveiled by APOGEE DR17
Volume 19, Issue 21 - article #1
E. Spitoni
,
F. Matteucci
,
R. Gratton
,
B. Ratcliffe
,
I. Minchev
,
G. Cescutti
https://arxiv.org/abs/2405.11025
MINCE II. Neutron capture elements
Volume 19, Issue 16 - article #6
P. Franc{c}ois
,
G. Cescutti
,
P. Bonifacio
,
E. Caffau
,
L. Monaco
,
M. Steffen
,
J. Puschnig
,
F. Calura
,
S. Cristallo
,
P. Di Marcantonio
,
V. Dobrovolskas
,
M. Franchini
,
A. J. Gallagher
,
C. J. Hansen
,
A. Korn
,
A. Kuvinskas
,
R. Lallement
,
L. Lombardo
,
F. Lucertini
,
L. Magrini
,
A. M. Matas Pinto
,
F. Matteucci
,
A. Mucciarelli
,
L. Sbordone
,
M. Spite
,
E. Spitoni
,
M. Valentini
https://arxiv.org/abs/2404.08418
Heavy element abundances in Galactic Globular Clusters
Volume 19, Issue 7 - article #6
J. Schiappacasse-Ulloa S. Lucatello G. Cescutti E. Carretta
https://arxiv.org/abs/2402.06490
Observational constraints on the origin of the elements. VIII. Constraining the Barium, Strontium and Yttrium chemical evolution in metal-poor stars. (arXiv:2311.05459v1 [astro-ph.SR])
Volume 18, Issue 44 - article #5
G. Guiglion
,
M. Bergemann
,
N. Storm
,
J. Lian
,
G. Cescutti
,
A. Serenelli
http://arxiv.org/abs/2311.05459
CUBES: a UV spectrograph for the future. (arXiv:2212.12791v1 [astro-ph.IM])
Volume 17, Issue 51 - article #1
S. Covino
,
S. Cristiani
,
J. M. Alcala'
,
S. H. P. Alencar
,
S. A. Balashev
,
B. Barbuy
,
N. Bastian
,
U. Battino
,
L. Bissell
,
P. Bristow
,
A. Calcines
,
G. Calderone
,
P. Cambianica
,
R. Carini
,
B. Carter
,
S. Cassisi
,
B. V. Castilho
,
G. Cescutti
,
N. Christlieb
,
R. Cirami
,
R. Conzelmann
,
I. Coretti
,
R. Cooke
,
G. Cremonese
,
K. Cunha
,
G. Cupani
,
A.R. da Silva
,
D. D'Auria
,
V. De Caprio
,
A. De Cia
,
H. Dekker
,
V. D'Elia
,
G. De Silva
,
M. Diaz
,
P. Di Marcantonio
,
V. D'Odorico
,
H. Ernandes
,
C. Evans
,
A. Fitzsimmons
,
M. Franchini
,
B. Gaensicke
,
M. Genoni
,
R. E. Giribaldi
,
C. Gneiding
,
A. Grazian
,
C. J. Hansen
,
J. Hopgood
,
J. Kosmalski
,
F. La Forgia
,
P. La Penna
,
M. Landoni
,
M. Lazzarin
,
D. Lunney
,
W. Maciel
,
W. Marcolino
,
M. Marconi
,
A. Migliorini
,
C. Miller
,
A. Modigliani
,
P. Noterdaeme
,
et al.
(29 additional authors not shown)
http://arxiv.org/abs/2212.12791
The cerium content of the Milky Way as revealed by Gaia DR3 GSP-Spec abundances. (arXiv:2207.05368v2 [astro-ph.GA] UPDATED)
Volume 17, Issue 49 - article #3
G. Contursi
,
P. de Laverny
,
A. Recio-Blanco
,
E.Spitoni
,
P. A. Palicio
,
E. Poggio
,
V. Grisoni
,
G. Cescutti
,
F. Matteucci
,
L. Spina
,
M. A. Alvarez
,
G. Kordopatis
,
C. Ordenovic
,
I. Oreshina-Slezak
,
H. Zhao
http://arxiv.org/abs/2207.05368
CUBES, the Cassegrain U-Band Efficient Spectrograph. (arXiv:2208.01672v1 [astro-ph.IM])
Volume 17, Issue 31 - article #3
S. Cristiani
,
J. M. Alcalá
,
S. H. P. Alencar
,
S. A. Balashev
,
N. Bastian
,
B. Barbuy
,
U. Battino
,
A. Calcines
,
G. Calderone
,
P. Cambianica
,
R. Carini
,
B. Carter
,
S. Cassisi
,
B. V. Castilho
,
G. Cescutti
,
N. Christlieb
,
R. Cirami
,
I. Coretti
,
R. Cooke
,
S. Covino
,
G. Cremonese
,
K. Cunha
,
G. Cupani
,
A. R. da Silva
,
V. De Caprio
,
A. De Cia
,
H. Dekker
,
V. D'Elia
,
G. De Silva
,
M.Diaz
,
P. Di Marcantonio
,
D. D'Auria
,
V. D'Odorico
,
A. Fitzsimmons
,
H. Ernandes
,
C. Evans
,
M. Franchini
,
M. Genoni
,
B. Gänsicke
,
R. E. Giribaldi
,
C. Gneiding
,
A. Grazian
,
C. J. Hansen
,
F. La Forgia
,
M. Landoni
,
M. Lazzarin
,
D. Lunney
,
W. Maciel
,
W. Marcolino
,
M.Marconi
,
A. Migliorini
,
C. Miller
,
P. Noterdaeme
,
C. Opitom
,
G. Pariani
,
B. Pilecki
,
S. Piranomonte
,
A. Quirrenbach
,
E.M.A. Redaelli
,
C. B. Pereira
,
et al.
(17 additional authors not shown)
http://arxiv.org/abs/2208.01672
The Gaia-ESO survey: placing constraints on the origin of r-process elements. (arXiv:2207.14747v1 [astro-ph.GA])
Volume 17, Issue 31 - article #10
M. Van der Swaelmen
,
C. Viscasillas Vázquez
,
G. Cescutti
,
L. Magrini
,
S. Cristallo
,
D. Vescovi
,
S. Randich
,
G. Tautvaišienė
,
V. Bagdonas
,
T. Bensby
,
M. Bergemann
,
A. Bragaglia
,
A. Drazdauskas
,
F. Jiménez-Esteban
,
G. Guiglion
,
A. Korn
,
T. Masseron
,
R. Minkevičiūtė
,
R. Smiljanic
,
L. Spina
,
E. Stonkutė
,
S. Zaggia
http://arxiv.org/abs/2207.14747
Simulated observations of heavy elements with CUBES. (arXiv:2203.15693v1 [astro-ph.IM])
Volume 17, Issue 13 - article #6
H. Ernandes
,
B. Barbuy
,
B. Castilho
,
C. J. Evans
,
G. Cescutti
http://arxiv.org/abs/2203.15693
Barium lines in high-quality spectra of two metal-poor giants in the Galactic halo. (arXiv:2109.00277v1 [astro-ph.SR])
Volume 16, Issue 36 - article #1
G. Cescutti
,
C. Morossi
,
M. Franchini
,
P. Di Marcantonio
,
C. Chiappini
,
M. Steffen
,
M. Valentini
,
P. François
,
N. Christlieb
,
C. Cortés
,
C. Kobayashi
,
E. Depagne
http://arxiv.org/abs/2109.00277
Stellar astrophysics in the near UV with VLT-CUBES. (arXiv:2102.02205v1 [astro-ph.IM])
Volume 16, Issue 6 - article #8
H. Ernandes
,
C. J. Evans
,
B. Barbuy
,
B. Castilho
,
G. Cescutti
,
N. Christlieb
,
S. Cristiani
,
G. Cupani
,
P. Di Marcantonio
,
M. Franchini
,
C. Hansen
,
A. Quirrenbach
,
R. Smiljanic
http://arxiv.org/abs/2102.02205
Neutron stars mergers in a stochastic chemical evolution model: impact of time delay distributions. (arXiv:2009.09534v1 [astro-ph.GA])
Volume 15, Issue 39 - article #6
L. Cavallo
,
G. Cescutti
,
F. Matteucci
http://arxiv.org/abs/2009.09534
Lithium in the closest satellite of our Milky Way. (arXiv:2004.06606v1 [astro-ph.SR])
Volume 15, Issue 16 - article #3
G. Cescutti
,
P. Molaro
,
X. Fu
http://arxiv.org/abs/2004.06606
Phosphorus Abundances in the Hyades and Galactic Disk
Volume 14, Issue 45 - article #10
Z. G. Maas
,
G. Cescutti,
,
C. A. Pilachowski
The Astronomical Journal
http://iopscience.iop.org/1538-3881/158/6/219
The CEMP star SDSS J0222–0313: the first evidence of proton ingestion in very low-metallicity AGB stars?★
Volume 14, Issue 32 - article #12
E. Caffau
,
L. Monaco
,
P. Bonifacio
,
S. Korotin
,
S. Andrievsky
,
S. Cristallo
,
M. Spite
,
F. Spite
,
L. Sbordone
,
P. François
,
G. Cescutti
,
S. Salvadori
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/hdWCxENgn8g/201935680
4MOST: Project overview and information for the First Call for Proposals. (arXiv:1903.02464v1 [astro-ph.IM])
Volume 14, Issue 10 - article #4
R.S. de Jong
,
O. Agertz
,
A. Agudo Berbel
,
J. Aird
,
D.A. Alexander
,
A. Amarsi
,
F. Anders
,
R. Andrae
,
B. Ansarinejad
,
W. Ansorge
,
P. Antilogus
,
H. Anwand-Heerwart
,
A. Arentsen
,
A. Arnadottir
,
M. Asplund
,
M. Auger
,
N. Azais
,
D. Baade
,
G. Baker
,
S. Baker
,
E. Balbinot
,
I.K. Baldry
,
M. Banerji
,
S. Barden
,
P. Barklem
,
E. Barthélémy-Mazot
,
C. Battistini
,
S. Bauer
,
C.P.M. Bell
,
O. Bellido-Tirado
,
S. Bellstedt
,
V. Belokurov
,
T. Bensby
,
M. Bergemann
,
J.M. Bestenlehner
,
R. Bielby
,
M. Bilicki
,
C. Blake
,
J. Bland-Hawthorn
,
C. Boeche
,
W. Boland
,
T. Boller
,
S. Bongard
,
A. Bongiorno
,
P. Bonifacio
,
D. Boudon
,
D. Brooks
,
M.J.I. Brown
,
R. Brown
,
M. Brüggen
,
J. Brynnel
,
J. Brzeski
,
T. Buchert
,
P. Buschkamp
,
E. Caffau
,
P. Caillier
,
J. Carrick
,
L. Casagrande
,
S. Case
,
A. Casey
,
I. Cesarini
,
G. Cescutti
,
et al.
(276 additional authors not shown)
http://arxiv.org/abs/1903.02464
The s-process nucleosynthesis in low mass stars: impact of the uncertainties in the nuclear physics determined by Monte Carlo variations. (arXiv:1810.04556v1 [astro-ph.SR])
Volume 13, Issue 41 - article #12
G. Cescutti
,
R. Hirschi
,
N. Nishimura
,
T. Rauscher
,
J. den Hartogh
,
A. St. J. Murphy
,
S. Cristallo
http://arxiv.org/abs/1810.04556
Uncertainties in s-process nucleosynthesis in low mass stars determined from Monte Carlo variations. (arXiv:1805.01250v1 [astro-ph.SR])
Volume 13, Issue 18 - article #23
G. Cescutti
,
R. Hirschi
,
N. Nishimura
,
J. W. den Hartogh
,
T. Rauscher
,
A. St. J. Murphy
,
S. Cristallo
http://arxiv.org/abs/1805.01250
Impacts of nuclear-physics uncertainties in the s-process determined by Monte-Carlo variations. (arXiv:1802.05836v1 [astro-ph.SR])
Volume 13, Issue 8 - article #5
N. Nishimura
,
G. Cescutti
,
R. Hirschi
,
T. Rauscher
,
J. den Hartogh
,
A. St. J. Murphy
http://arxiv.org/abs/1802.05836
The s-process nucleosynthesis: impact of the uncertainties in the nuclear physics determined by Monte Carlo variations. (arXiv:1708.01629v1 [astro-ph.SR])
Volume 12, Issue 32 - article #6
G. Cescutti
,
N. Nishimura
,
R. Hirschi
,
T. Rauscher
,
J. W. den Hartogh
,
A. St. J. Murphy
http://arxiv.org/abs/1708.01629
Phosphorus Abundances in FGK Stars
Volume 12, Issue 22 - article #8
Z. G. Maas
,
C. A. Pilachowski,
,
G. Cescutti
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/841/2/108
Abundances of carbon-enhanced metal-poor stars as constraints on their formation
Volume 10, Issue 43 - article #2
C.J. Hansen
,
B. Nordstroem
,
T.T. Hansen
,
C.R. Kennedy
,
V.M. Placco
,
T.C. Beers
,
J. Andersen
,
G. Cescutti
,
C. Chiappini
arXiv.org - Astrophysics - Volume: 2015, Issue: 20 Nov
arXiv:1511.07812
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The role of neutron star mergers in the chemical evolution of the Galactic halo
Volume 10, Issue 10 - article #14
G. Cescutti
,
D. Romano
,
F. Matteucci
,
C. Chiappini
,
R. Hirschi
arXiv.org - Astrophysics - Volume: 2015, Issue: 13 Mar
arXiv:1503.02954
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High-resolution abundance analysis of red giants in the globular cluster NGC 6522
Volume 9, Issue 24 - article #40
B. Barbuy
,
C. Chiappini
,
E. Cantelli
,
E. Depagne
,
M. Pignatari
,
R. Hirschi
,
G. Cescutti
,
S. Ortolani
,
V. Hill
,
M. Zoccali
,
et al.
(4 more)
D. Minniti
,
M. Trevisan
,
E. Bica
and
A. Gómez
Astronomy and Astrophysics - Volume: 570, Issue: October 2014
http://dx.doi.org/10.1051/0004-6361/201424311
Abstract
Full HTML
PDF (1.165 MB)
ePUB (2.306 MB)
References
Online Material
SIMBAD record
NASA ADS Abstract Service
High-resolution abundance analysis of red giants in the globular cluster NGC 6522
Volume 9, Issue 21 - article #11
B. Barbuy
,
C. Chiappini
,
E. Cantelli
,
E. Depagne
,
M. Pignatari
,
R. Hirschi
,
G. Cescutti
,
S. Ortolani
,
V. Hill
,
M. Zoccali
,
D. Minniti
,
M. Trevisan
,
E. Bica
,
A. Gómez
arXiv.org - Astrophysics - Volume: 2014, Issue: 15 Aug
arXiv:1408.2438
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Explaining the Ba, Y, Sr, and Eu abundance scatter in metal-poor halo stars: constraints to the r-process
Volume 9, Issue 21 - article #35
G. Cescutti
and
C. Chiappini
Astronomy and Astrophysics - Volume: 565, Issue: May 2014
http://dx.doi.org/10.1051/0004-6361/201423432
Abstract
Full HTML
PDF (3.293 MB)
ePUB (1.707 MB)
References
Online Material
NASA ADS Abstract Service
The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe?
Volume 8, Issue 23 - article #16
G. Cescutti
,
C. Chiappini
,
R. Hirschi
,
G. Meynet
and
U. Frischknecht
Astronomy and Astrophysics - Volume: 553, Issue: May 2013
http://dx.doi.org/10.1051/0004-6361/201220809
Abstract
Full HTML
PDF (1.245 MB)
References
Online Material
NASA ADS Abstract Service
LTE or non-LTE, that is the question - The NLTE chemical evolution of strontium in extremely metal-poor stars
Volume 8, Issue 11 - article #8
C. J. Hansen
,
M. Bergemann
,
G. Cescutti
,
P. François
,
A. Arcones
,
A. I. Karakas
,
K. Lind
and
C. Chiappini
Astronomy and Astrophysics - Volume: 551, Issue: March 2013
http://dx.doi.org/10.1051/0004-6361/201220584
Abstract
Full HTML
PDF (522.2 KB)
References
NASA ADS Abstract Service
Chemical evolution of the Galactic bulge: different stellar populations and possible gradients
Volume 7, Issue 51 - article #80
V. Grieco
,
F. Matteucci
,
A. Pipino
and
G. Cescutti
Astronomy and Astrophysics - Volume: 548, Issue: December 2012
http://dx.doi.org/10.1051/0004-6361/201219761
Abstract
|
Full HTML
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PDF (234.7 KB)
|
References
|
NASA ADS Abstract Service
Chemical evolution of the Galactic bulge: different stellar populations and possible gradients
Volume 7, Issue 38 - article #2
V. Grieco
,
F. Matteucci
,
A. Pipino
,
G. Cescutti
arXiv.org - Astrophysics - Volume: 2012, Issue: 21 Sep
arXiv:1209.4462
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The evolution of carbon and oxygen in the bulge and disk of the Milky Way
Volume 4, Issue 41 - article #29
G. Cescutti
,
F. Matteucci
,
A. McWilliam
,
and
C. Chiappini
Astronomy and Astrophysics - Volume: 505, Issue: 2
Abstract
|
PDF file (214.1 KB)
|
PS file (115.4 KB)
Effects of galactic fountains and delayed mixing in the chemical evolution of the Milky Way
Volume 4, Issue 37 - article #19
E. Spitoni
,
F. Matteucci
,
S. Recchi
,
G. Cescutti
,
and
A. Pipino
Astronomy and Astrophysics - Volume: 504, Issue: 1
Abstract
|
Full HTML
|
PDF file (653.4 KB)
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PS file (305.5 KB)
|
References
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Original article
Effects of Galactic fountains and delayed mixing in the chemical evolution of the Milky Way
Volume 4, Issue 25 - article #5
E. Spitoni
(1),
F. Matteucci
(1,2),
S. Recchi
(3,2),
G. Cescutti
(1),
A. Pipino
(4)
((1) Dipartimento di Astronomia, Universita' di Trieste, Italy,
(2) I.N.A.F. Osservatorio Astronomico di Trieste, Italy,
(3) Institute of Astronomy, Vienna University, Austria
(4) Department of Physics and Astronomy, University of Southern California, U.S.A)
arXiv.org - Astrophysics - Volume: 2009, Issue: 19 Jun
arXiv:0906.3400
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other
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The origin of abundance gradients in the Milky Way: the predictions of different models
Volume 4, Issue 12 - article #28
E. Colavitti
,
G. Cescutti
,
F. Matteucci
,
and
G. Murante
Astronomy and Astrophysics - Volume: 496, Issue: 2
Abstract
|
PDF file (313.1 KB)
|
PS file (249.5 KB)
The origin of abundance gradients in the Milky Way: the predictions of different models
Volume 3, Issue 48 - article #10
E. Colavitti
,
G. Cescutti
,
F. Matteucci
,
G. Murante
arXiv.org - Astrophysics - Volume: 2008, Issue: 27 Nov
arXiv:0811.3505
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The chemical evolution of Manganese in different stellar systems
Volume 3, Issue 28 - article #15
G. Cescutti
,
F. Matteucci
,
G.A. Lanfranchi
,
A. McWilliam
arXiv.org - Astrophysics - Volume: 2008, Issue: 10 Jul
arXiv:0807.1463
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The Evolution of Oxygen and Magnesium in the Bulge and Disk of the Milky Way
Volume 3, Issue 25 - article #22
<em >A. McWilliam
,
F. Matteucci
,
S. Ballero
,
R. M. Rich
,
J. P. Fulbright
,
and
G. Cescutti</em>
,
Astronomical Journal - Volume: 136, Issue: 1
Abstract
|
References
A comparison of the
s
- and
r
-process element evolution in local dwarf spheroidal galaxies and in the Milky Way
Volume 3, Issue 14 - article #9
G. A. Lanfranchi
,
F. Matteucci
,
and
G. Cescutti
Astronomy and Astrophysics - Volume: 481, Issue: 3
Abstract
|
PDF file (531.8 KB)
|
PS file (144.2 KB)
An inhomogeneous model for the Galactic halo: a possible explanation for the spread observed in
s
- and
r
-process elements
Volume 3, Issue 14 - article #10
G. Cescutti
Astronomy and Astrophysics - Volume: 481, Issue: 3
Abstract
|
PDF file (1.653 MB)
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PS file (785.9 KB)
An inhomogeneous model for the Galactic halo: a possible explanation for the spread observed in s- and r-process elements
Volume 3, Issue 6 - article #7
G. Cescutti
(Astronomy Department, Trieste University)
arXiv.org - Astrophysics - Volume: 2008, Issue: 7 Feb
arXiv:0802.0678
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The Evolution of Oxygen and Magnesium in the Bulge and Disk of the Milky Way
Volume 2, Issue 35 - article #14
A. McWilliam
,
F. Matteucci
,
S. Ballero
,
R.M. Rich
,
J. P. Fulbright
,
G. Cescutti
ArXiv - Astrophysics
arXiv:0708.4026
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other
]
Detailed chemical evolution of Carina and Sagittarius dwarf spheroidal galaxies
Volume 1, Issue 21 - article #14
G. A. Lanfranchi
,
F. Matteucci
and
G. Cescutti
Astronomy and Astrophysics - Volume 453, Issue 1 - June, 2006
Abstract
, Full HTML,
PDF file (208 KB)
,
PS file (77.6 KB)
, References
The chemical evolution of barium and europium in the Milky Way
Volume 1, Issue 6 - article #17
G. Cescutti
,
P. François
,
F. Matteucci
,
R. Cayrel
and
M. Spite
Astronomy and Astrophysics - Volume 448, Issue 2 - February, 2006
Abstract
,
PDF file (461 KB)
,
PS file (329 KB)
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