The formation of hot subdwarf stars and its implications for the UV-upturn phenomenon of elliptical...
The formation of hot subdwarf stars and its implications for the UV-upturn phenomenon of elliptical galaxies
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Publisher
Dordrecht: Springer Netherlands
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Language
English
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Dordrecht: Springer Netherlands
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In this paper, we review the formation scenario for field hot subdwarf stars and extreme horizontal branch stars in globular clusters and discuss how the scenario helps us to understand the UV-upturn phenomenon of elliptical galaxies.
It is widely accepted that field hot subdwarf stars originate from binary evolution via the following three chan...
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Full title
The formation of hot subdwarf stars and its implications for the UV-upturn phenomenon of elliptical galaxies
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TN_cdi_proquest_journals_775461393
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_775461393
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ISSN
0004-640X
E-ISSN
1572-946X
DOI
10.1007/s10509-010-0348-4
