Analysis of the spectral energy distributions of four cool R CrB stars near the brightness maximum
Analysis of the spectral energy distributions of four cool R CrB stars near the brightness maximum
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Author / Creator
Publisher
Boston: Springer US
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Language
English
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Publisher
Boston: Springer US
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Scope and Contents
Contents
The effective temperatures
T
eff
and carbon and nitrogen abundances in the atmospheres of the cool R CrB stars ES Aql, SV Sge, Z UMi, and NSV 11154 have been determined by modeling their spectral energy distributions in the optical and near-infrared. The hydrogen-deficient model atmospheres were computed using the SAM12 code in the classic...
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Full title
Analysis of the spectral energy distributions of four cool R CrB stars near the brightness maximum
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Record Identifier
TN_cdi_proquest_miscellaneous_1448221930
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1448221930
Other Identifiers
ISSN
1063-7729
E-ISSN
1562-6881
DOI
10.1134/S1063772913100077
