Pulsational Evidence for Mass Loss in NGC 1866 Cepheids
- 1 October 2004
- journal article
- Published by American Astronomical Society in The Astronomical Journal
- Vol. 128 (4), 1597-1605
- https://doi.org/10.1086/423917
Abstract
No abstract availableThis publication has 20 references indexed in Scilit:
- Stellar evolutionary models for Magellanic CloudsAstronomy & Astrophysics, 2003
- The Luminosity Function of the Large Magellanic Cloud Globular Cluster NGC 1866The Astronomical Journal, 2003
- Distance to the Large Magellanic Cloud: The RR Lyrae StarsThe Astronomical Journal, 2003
- Improving the Mass Determination of Galactic CepheidsThe Astrophysical Journal, 2001
- Cepheid mass-luminosity relations from the Magellanic CloudsAstronomy & Astrophysics, 2001
- Distances, Ages, and Epoch of Formation of Globular ClustersThe Astrophysical Journal, 2000
- Classical Cepheid Pulsation Models. III. The Predictable ScenarioThe Astrophysical Journal, 2000
- Theoretical Models for Classical Cepheids. II. Period‐Luminosity, Period‐Color, and Period‐Luminosity‐Color RelationsThe Astrophysical Journal, 1999
- Analysis of Stellar Content and Cepheid Evolution in NGC 1866The Astrophysical Journal, 1967
- The Star Cluster NGC 1866 and its CepheidsThe Astrophysical Journal, 1967