The chemical composition of donors in AM CVn stars and ultracompact X-ray binaries: observational tests of their formation
- Author
- NELEMANS, G1 ; YUNGELSON, L. R1 2 ; VAN DER SLUYS, M. V3 ; TOUT, Christopher A4
[1] Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, Netherlands
[2] Institute of Astronomy of the Russian Academy of Sciences, 48 Pyatnitskaya Str., 119017 Moscow, Russian Federation
[3] Department of Astrophysics, Northwestern University, Evanston, IL 60208, United States
[4] Institute of Astronomy University of Cambridge, Madingley Road, Cambridge CB3 OHA, United Kingdom - Source
Monthly notices of the Royal Astronomical Society (Print). 2010, Vol 401, Num 2, pp 1347-1359, 13 p ; ref : 1 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Wiley-Blackwell, Malden, MA
- Publication country
- United States
- Document type
- Article
- Language
- Russian
- Author keyword
- binaries: close stars: evolution white dwarfs
- Keyword (fr)
- Abondance Binaire RX Binaire serrée Combustion hélium Composition chimique Etoile hélium Etoile naine Etoile séquence principale Evolution stellaire Naine blanche Rapport carbone oxygène Source RX binaire Source RX cosmique Transfert masse
- Keyword (en)
- Abundance X-ray binary stars Close binary stars Helium burning Chemical composition Helium stars Dwarf stars Main sequence stars Stellar evolution White dwarf stars Carbon oxygen ratio Binary X ray source Cosmic x-ray sources Mass transfer
- Keyword (es)
- Relación carbono oxígeno Fuente RX binaria
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 22280206
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
10.1111/j.1365-2966.2009.15731.x 
https://dx.doi.org/10.1111/j.1365-2966.2009.15731.x
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