Constraining the X-ray luminosities of asymptotic giant branch stars: TX camelopardalis and T cassiopeia
- Author
- KASTNER, Joel H1 ; SOKER, Noam2
[1] Chester F. Carlson Center for Imaging Science, Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623, United States
[2] Department of Physics, Technion-Israel Institute of Technology, Haifa 32000, Israel - Source
The Astrophysical journal. 2004, Vol 608, Num 2, pp 978-982, 5 p ; 1 ; ref : 35 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)
- Branche géante asymptotique Champ magnétique Emission RX Luminosité Observation RX Perte masse Vent stellaire
- Keyword (en)
- Asymptotic giant branch Magnetic fields X ray emission Luminosity X ray observation Mass loss Stellar winds
- Keyword (es)
- Rama gigante asintótica Emisión RX Observación RX
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10L Magnetic and electric fields. Polarization of starlight
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10M Mass loss and stellar winds
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C20 Normal stars (by class): general or individual / 001E03C20L Giant and subgiant stars
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 15997844
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
10.1086/420877 
https://dx.doi.org/10.1086/420877
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