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THE PULSATIONAL PROPERTIES OF HIGH-LUMINOSITY DEGENERATE STARS WITH HYDROGEN BURNING NEAR THE SURFACE.

Author
VILA SC; SION EM
DEP. ASTRON., UNIV. PENNSYLVANIA, PHILADELPHIA, PA. 19184
Source
ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 207; NO 3 PART. 1; PP. 820-823; BIBL. 20 REF.
Document type
Article
Language
English
Keyword (fr)
ETOILE DEGENEREE PULSATION STELLAIRE EVOLUTION STELLAIRE MODELE INSTABILITE STELLAIRE PULSATION RADIALE ASTRONOMIE
Keyword (en)
DEGENERATE STAR STELLAR PULSATION STELLAR EVOLUTION MODELS STELLAR INSTABILITY RADIAL PULSATION ASTRONOMY
Keyword (es)
ASTRONOMIA
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
PASCAL7730026378

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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