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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DOI
10.1086/422905 
https://dx.doi.org/10.1086/422905
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