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SEISMOLOGICAL ANALYSIS OF THE STARS γ SERPENTIS AND τ LEONIS : STELLAR PARAMETERS AND EVOLUTION

Author
BI, S.-L1 2 ; BASU, Sarbani3 ; LI, L.-H3
[1] Department of Astronomy, Beijing Normal University, 100875 Beijing, China
[2] National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011 Yunnan, China
[3] Department of Astronomy, Yale University, New Haven, CT 06520, United States
Source

The Astrophysical journal. 2008, Vol 673, Num 2, pp 1093-1105, 13 p ; 1 ; ref : 1/2 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
stars: evolution stars: fundamental parameters stars: individual (γ Serpentis = HD 142860, τ Leonis = HD 99028) stars: oscillations
Keyword (fr)
Evolution stellaire Paramètre physique
Keyword (en)
Stellar evolution Physical parameter
Keyword (es)
Parámetro físico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20056305

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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