Formation of the dark bays in the Crab optical synchrotron nebula : is the Crab pulsar wind bubble interacting with its progenitor's wind ?
- Author
- ZHI-YUN LI; BEGELMAN, M. C
Univ. Colorado, joint inst. lab. astrophysics, Boulder CO 80309-0440, United States - Source
The Astrophysical journal. 1992, Vol 400, Num 1, pp 186-191 ; 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)
- Bulle interstellaire Cinématique Emission RX Formation Magnétohydrodynamique Modèle Mécanisme rayonnement Nébuleuse Crabe Pulsar Rayonnement cyclotron Rayonnement synchrotron Vent stellaire
- Keyword (en)
- Interstellar bubble Kinematics X ray emission Formation Magnetohydrodynamics Models Radiation mechanism Crab nebula Pulsar Cyclotron radiation Synchrotron radiation Stellar wind
- Keyword (es)
- Burbuja interestelar Cinemática Emisión RX Formación Magnetohidrodinámica Modelo Mecanismo radiación Nebulosa Crabe Pulsar Radiación ciclotrón Radiación sincrotrón Viento estelar
- 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
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 4412700
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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