Virtual Journal of Nuclear Astrophysics
Edited by
Honey Arora
, Michigan State University and
Fry Fang
, University of Notre Dame
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Results 1 - 9 of 9
Titanium abundances in late-type stars, II. Grid of departure coefficients and application to a sample of $70,000$ stars
Virtual Journal - Volume 22, Issue 13 - article #15
J. W. E. Mallinson
,
K. Lind
,
A. M. Amarsi
,
K. Youakim
https://arxiv.org/abs/2403.19304
Higher metal abundances do not solve the solar problem
Virtual Journal - Volume 21, Issue 2 - article #6
G. Buldgen
,
P. Eggenberger
,
A. Noels
,
R. Scuflaire
,
A. M. Amarsi
,
N. Grevesse
,
S. Salmon
Astronomy & Astrophysics
https://www.aanda.org/10.1051/0004-6361/202245448
The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines. (arXiv:2109.04752v1 [astro-ph.SR])
Virtual Journal - Volume 19, Issue 38 - article #8
A. M. Amarsi
,
N. Grevesse
,
M. Asplund
,
R. Collet
http://arxiv.org/abs/2109.04752
3D non-LTE line formation of neutral carbon in the Sun. (arXiv:1903.08838v1 [astro-ph.SR])
Virtual Journal - Volume 17, Issue 12 - article #1
A. M. Amarsi
,
P. S. Barklem
,
R. Collet
,
N. Grevesse
,
M. Asplund
http://arxiv.org/abs/1903.08838
Carbon and oxygen in metal-poor halo stars⋆
Virtual Journal - Volume 17, Issue 5 - article #5
A. M. Amarsi
,
P. E. Nissen
,
M. Asplund
,
K. Lind
,
P. S. Barklem
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/QTipYx6aF8Y/201834480
The GALAH Survey: Second Data Release. (arXiv:1804.06041v1 [astro-ph.SR])
Virtual Journal - Volume 16, Issue 16 - article #6
S. Buder
(1,2),
M. Asplund
(3,4),
L. Duong
(3),
J. Kos
(5),
K. Lind
(1,6),
M. K. Ness
(7,8),
S. Sharma
(5,4),
J. Bland-Hawthorn
(5,4),
A. R. Casey
(9),
G. M. De Silva
(10,5),
V. D'Orazi
(11),
K. C. Freeman
(3),
G. F. Lewis
(5),
J. Lin
(3,4),
S. L. Martell
(12),
K. J. Schlesinger
(3),
J. D. Simpson
(10),
D. B. Zucker
(13,10),
T. Zwitter
(14),
A. M. Amarsi
(1),
B. Anguiano
(15),
D. Carollo
(16),
K. Cotar
(14),
P. L. Cottrell
(9,17),
G. Da Costa
(3),
X. D. Gao
(1),
M. R. Hayden
(5,4),
J. Horner
(18),
M. J. Ireland
(3),
P. R. Kafle
(19),
U. Munari
(20),
D. M. Nataf
(21),
T. Nordlander
(3,4),
Dennis Stello
(12,22,4),
Y.-S. Ting
(23,24,25),
G. Traven
(14),
F. Watson
(10,26),
R. A. Wittenmyer
(18),
R. F. G. Wyse
(21),
D. Yong
(3),
J. C. Zinn
(27),
M. Zerjal
(3)
((1) MPIA Heidelberg,
(2) IMPRS HD,
(3) RSAA/MSO Canberra,
(4) ASTRO-3D Australia,
(5) SIfA Sydney,
(6) Uppsala University,
(7) Columbia University New York,
(8) CCA New York
(9) Monash University,
(10) AAO North Ryde,
(11) INAF Padova,
(12) UNSW Sydney,
(13) Macquarie University Sydney,
(14) University of Ljubljana,
(15) University of Virginia,
(16) INAF Turin,
(17) University of Canterbury,
(18) University of Southern Queensland,
(19) University of Western Australia,
(20) INAF Padova,
(21) Johns Hopkins University Baltimore,
(22) Aarhus University,
(23) IAS Princeton,
(24) Princeton University,
(25) Carnegie Observatories Pasadena,
(26) Western Sydney University,
(27) The Ohio State University)
http://arxiv.org/abs/1804.06041
The solar silicon abundance based on 3D non-LTE calculations. (arXiv:1609.07283v1 [astro-ph.SR])
Virtual Journal - Volume 14, Issue 40 - article #16
A. M. Amarsi
,
M. Asplund
http://arxiv.org/abs/1609.07283
Non-LTE line formation of Fe in late-type stars - III. 3D non-LTE analysis of metal-poor stars. (arXiv:1608.06390v1 [astro-ph.SR])
Virtual Journal - Volume 14, Issue 35 - article #11
A. M. Amarsi
,
K. Lind
,
M. Asplund
,
P. S. Barklem
,
R. Collet
http://arxiv.org/abs/1608.06390
On line contribution functions and examining spectral line formation in 3D model stellar atmospheres
Virtual Journal - Volume 13, Issue 28 - article #15
A. M. Amarsi
Monthly Notices of the Royal Astronomical Society - Volume: 452, Issue: 2
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