Hot Subdwarf Stars
Hot Subdwarf Stars
About this item
Full title
Hot Subdwarf Stars
Author / Creator
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
arXiv.org, 2024-10
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
Hot subdwarf (SD) stars are the stripped cores of red giant stars in transition to the white dwarf sequence. The B-type subdwarfs (sdB) are powered by helium fusion in the core, more evolved ones (sdO) by shell burning. Low mass SDs may evolve through this stage without any support by nuclear fusion. Because the loss of the giants' envelopes is lik...
Alternative Titles
Full title
Hot Subdwarf Stars
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_3117168829
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3117168829
Other Identifiers
E-ISSN
2331-8422
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