Author:
Briley Michael M.,Cohen Judith G.,Stetson Peter B.
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
55 articles.
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1. Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si − III. Grids of isochrones for −2.5 ≤ [Fe/H] ≤ −0.5 and helium abundances Y = 0.25 and 0.29 at each metallicity;Monthly Notices of the Royal Astronomical Society;2022-11-11
2. BACCHUS Analysis of Weak Lines in APOGEE Spectra (BAWLAS);The Astrophysical Journal Supplement Series;2022-09-01
3. Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si. II. Application to the colour–magnitude diagrams of the globular clusters 47 Tuc, NGC 6362, M 5, M 3, M 55, and M92;Monthly Notices of the Royal Astronomical Society;2021-10-21
4. Models of metal-poor stars with different initial abundances of C, N, O, Mg, and Si – I. Bolometric corrections derived from new MARCS synthetic spectra and their implications for observed colour–magnitude diagrams;Monthly Notices of the Royal Astronomical Society;2021-10-21
5. Light Element Abundances and Multiple Populations in M53;The Astronomical Journal;2021-05-28