A semi-empirical study of the mass distribution of horizontal branch stars in M 3 (NGC 5272)
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20078231/pdf
Reference41 articles.
1. Detecting bimodality in astronomical datasets
2. Synthetic Mean Colors for RR Lyrae Variables
3. A Multicolor and Fourier Study of RR Lyrae Variables in the Globular Cluster NGC 5272 (M3)
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1. Multiwavelength photometric study of RR lyrae variables in the globular cluster NGC 5272 (Messier 3);Monthly Notices of the Royal Astronomical Society;2024-05-24
2. Red horizontal branch stars: An asteroseismic perspective;Astronomy & Astrophysics;2023-03
3. The SDSS-Gaia View of the Color–Magnitude Relation for Blue Horizontal-branch Stars;The Astrophysical Journal;2022-11-01
4. Evolution and Period Change in RR Lyr Variables of the Globular Cluster M 3;Astronomy Letters;2018-10
5. Constraints on the Distance Moduli, Helium, and Metal Abundances, and Ages of Globular Clusters from Their RR Lyrae and Non-variable Horizontal Branch Stars. II. Multiple Stellar Populations in 47 Tuc, M3, and M13;The Astrophysical Journal;2017-11-10
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