Gauging the Helium Abundance of the Galactic Bulge RR Lyrae Stars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/aaa8e3/pdf
Reference38 articles.
1. Metal‐rich RR Lyrae Variables. II. The Pulsational Scenario
2. Metal abundances of RR Lyrae variables in selected galactic star fields. I - Baade's window
3. The relationship between infrared, optical, and ultraviolet extinction
4. The Initial Helium Content of Galactic Globular Cluster Stars from theR‐Parameter: Comparison with the Cosmic Microwave Background Constraint
5. VVV SURVEY NEAR-INFRARED PHOTOMETRY OF KNOWN BULGE RR LYRAE STARS: THE DISTANCE TO THE GALACTIC CENTER AND ABSENCE OF A BARRED DISTRIBUTION OF THE METAL-POOR POPULATION
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2. RR Lyrae from binary evolution: abundant, young, and metal-rich;Monthly Notices of the Royal Astronomical Society;2023-12-23
3. Near-infrared observations of RR Lyrae and Type II Cepheid variables in the metal-rich bulge globular cluster NGC 6441;Astronomy & Astrophysics;2022-12
4. RR Lyrae Stars and Anomalous Cepheids as Population Tracers in Local Group Galaxies;Universe;2022-03-19
5. RR Lyrae and Type II Cepheid Variables in Globular Clusters: Optical and Infrared Properties;Universe;2022-02-13
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