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Mass-radius constraints from a pulse shape model for Hercules X-1

Author
LEAHY, D. A1
[1] Department of Physics and Astronomy, University of Calgary, Calgary, AB T2N 1N4, Canada
Source

The Astrophysical journal. 2004, Vol 613, Num 1, pp 517-521, 5 p ; 1 ; ref : 21 ref

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
Keyword (fr)
Accrétion stellaire Binaire RX Binaire serrée Etoile neutron Forme impulsion Modèle Relation masse rayon Source RX binaire Source RX cosmique
Keyword (en)
Star accretion X-ray binary stars Close binary stars Neutron stars Pulse shape Models Mass radius relation Binary X ray source Cosmic x-ray sources
Keyword (es)
Forma impulsión Modelo Relación masa radio Fuente RX binaria
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C60 Late stages of stellar evolution (including black holes) / 001E03C60J Neutron stars

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C80 Binary and multiple stars / 001E03C80J X-ray binaries

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16227265

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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