Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. III. M55 and NGC 6362-Reference-Cited by-同舟云学术

Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. III. M55 and NGC 6362

Published:2018-07-24 Issue:1 Volume:862 Page:72
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

VandenBerg Don A.^ORCID,Denissenkov P. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/862/i=1/a=72/pdf

Reference142 articles.

1. Non-LTE line formation of Fe in late-type stars – III. 3D non-LTE analysis of metal-poor stars

2. GALACTIC GLOBULAR AND OPEN CLUSTERS IN THE SLOAN DIGITAL SKY SURVEY. II. TEST OF THEORETICAL STELLAR ISOCHRONES

3. Metallicity and distance of NGC 6362 from its RR Lyrae and SX Phoenicis stars

4. RR Lyrae stars and the horizontal branch of NGC 5904 (M5)

5. The Globular Cluster M5.

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