Metal‐rich RR Lyrae Variables. I. The Evolutionary Scenario-Reference-Cited by-同舟云学术

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Metal‐rich RR Lyrae Variables. I. The Evolutionary Scenario

Published:1997-04-10 Issue:1 Volume:479 Page:279-289
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Bono Giuseppe,Caputo Filippina,Cassisi Santi,Castellani Vittorio,Marconi Marcella

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/479/i=1/a=279/pdf

Reference41 articles.

1. Low-temperature Rosseland opacities

2. Bono, G., Caputo, F., Castellani V. & Marconi M. 1996, A&AS, in press

3. Bono, G., Caputo, F., Cassisi, S. & Marconi, M. 1997a, ApJ, submitted

4. Bono, G., Caputo, F., Cassisi, S. & Marconi, M. 1997b, in preparation

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1. RR Lyrae from binary evolution: abundant, young, and metal-rich;Monthly Notices of the Royal Astronomical Society;2023-12-23

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3. An Old, Metal-rich Accreted Stellar Component in the Milky Way Stellar Disk;The Astrophysical Journal;2022-07-01

4. RR Lyrae and Type II Cepheid Variables in Globular Clusters: Optical and Infrared Properties;Universe;2022-02-13

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