Journal
ASTROPHYSICS AND SPACE SCIENCE
Volume 291, Issue 3-4, Pages 205-213Publisher
KLUWER ACADEMIC PUBL
DOI: 10.1023/B:ASTR.0000044323.22830.35
Keywords
UV upturn; galaxy evolution; sdB stars; EHB stars
Categories
Ask authors/readers for more resources
The UV upturn phenomenon found in bright elliptical galaxies has notable implications for stellar evolution, galaxy evolution and even for cosmology. The recent space observations of three galaxy clusters made by Brown and his collaborators shed great lights on this field of study. Theoretical models are being improved based on such data. While the core-helium burning stars remain the strongest candidate for the UV upturn, there is a growing concern that the canonical models may be missing important elements, such as binaries. I review the current theoretical understanding and future prospects.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available