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, University of Notre Dame
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Results 1 - 5 of 5
Metallicity distributions of halo stars: do they trace the Galactic accretion history?. (arXiv:2401.13737v1 [astro-ph.GA])
Volume 19, Issue 4 - article #7
A. Mori
,
P. Di Matteo
,
S. Salvadori
,
S. Khoperskov
,
G. Pagnini
,
M. Haywood
http://arxiv.org/abs/2401.13737
StarHorse results for spectroscopic surveys with Gaia EDR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars (Corrigendum)⋆
Volume 18, Issue 34 - article #5
A. B. A. Queiroz
,
F. Anders
,
C. Chiappini
,
A. Khalatyan
,
B. X. Santiago
,
S. Nepal
,
M. Steinmetz
,
C. Gallart
,
M. Valentini
,
M. Dal Ponte
,
B. Barbuy
,
A. Pérez-Villegas
,
T. Masseron
,
J. G. Fernández-Trincado
,
S. Khoperskov
,
I. Minchev
,
E. Fernández-Alvar
,
R. R. Lane
,
C. Nitschelm
Astronomy & Astrophysics
https://www.aanda.org/10.1051/0004-6361/202245399e
Revisiting long-standing puzzles of the Milky Way: the Sun and its vicinity as typical outer disk chemical evolution. (arXiv:1903.03188v1 [astro-ph.GA])
Volume 14, Issue 11 - article #4
M. Haywood
,
O. N. Snaith
,
M. D. Lehnert
,
P. Di Matteo
,
S. Khoperskov
http://arxiv.org/abs/1903.03188
The Milky Way has no in-situ halo but it has a thick disc. Composition of the stellar halo and age-dating the last significant merger with Gaia DR2 and APOGEE. (arXiv:1812.08232v1 [astro-ph.GA])
Volume 13, Issue 51 - article #6
P. Di Matteo
,
M. Haywood
,
M. D. Lehnert
,
D. Katz
,
S. Khoperskov
,
O. N. Snaith
,
A. Gómez
,
N. Robichon
http://arxiv.org/abs/1812.08232
What the Milky Way bulge reveals about the initial metallicity gradients in the disc
Volume 12, Issue 45 - article #10
F. Fragkoudi
,
P. Di Matteo
,
M. Haywood
,
S. Khoperskov
,
A. Gomez
,
M. Schultheis
,
F. Combes
,
B. Semelin
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/gAKjmtmm7x4/201731597
Results 1 - 5 of 5
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