On the Observational Properties of He‐burning Stars: Some Clues on the Tilt of the Horizontal Branch in Metal‐rich Clusters
- 20 April 2002
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 569 (2) , 975-983
- https://doi.org/10.1086/339428
Abstract
No abstract availableKeywords
All Related Versions
This publication has 31 references indexed in Scilit:
- Flash Mixing on the White Dwarf Cooling Curve: Understanding Hot Horizontal Branch Anomalies in NGC 2808The Astrophysical Journal, 2001
- The Color‐Magnitude Diagram of the Globular Cluster NGC 6362 and the Canonical Tilt of Horizontal BranchesThe Astrophysical Journal, 1999
- Galactic globular cluster stars: From theory to observationAstronomy and Astrophysics Supplement Series, 1999
- An updated theoretical scenario for globular cluster starsAstronomy and Astrophysics Supplement Series, 1998
- The Age of Globular Clusters in Light ofHipparcos: Resolving the Age Problem?The Astrophysical Journal, 1998
- Evolutionary and Pulsational Constraints for Super–Metal‐rich Stars withZ= 0.04The Astrophysical Journal, 1997
- Ultraviolet Radiation from Evolved Stellar Populations. I. ModelsThe Astrophysical Journal, 1993
- The relationship between infrared, optical, and ultraviolet extinctionThe Astrophysical Journal, 1989
- Theoretical models for helium-burning stars in intermediate-metallicity globular clustersThe Astrophysical Journal, 1989
- The effective temperatures and colours of G and K starsMonthly Notices of the Royal Astronomical Society, 1989