RADIO-TO-TeV PHASE-RESOLVED EMISSION FROM THE CRAB PULSAR: THE ANNULAR GAP MODEL
- Author
- DU, Y. J1 ; QIAO, G. J2 ; WANG, W1
[1] National Astronomical Observatories, Chinese Academy of Sciences, Jia 20 Datun Road, Beijing 100012, China
[2] School of Physics, Peking University, Beijing 100871, China - Source
The Astrophysical journal. 2012, Vol 748, Num 2 ; 84.1-84.12 ; 1 ; ref : 1/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- IOP, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- X-rays: individual (PSR B0531+21) acceleration of particles gamma rays: stars pulsars: general pulsars: individual (Crab: PSR B0531+21) radiation mechanisms: non-thermal
- Keyword (fr)
- Accélération particule Angle observation Champ électrique Courbe lumière Diffusion Compton inverse Domaine énergie TeV Emission particule Etoile neutron Loi normale Modèle Mécanisme rayonnement Observatoire spatial Particule chargée Particule secondaire Potentiel champ Potentiel électrique Pulsar Rapport signal bruit Rayon X mou Rayonnement courbure Rayonnement gamma Rayonnement synchrotron
- Keyword (en)
- Particle acceleration Viewing angle Electric fields Light curves Inverse Compton scattering TeV range Particle emission Neutron stars Normal distribution Models Radiation mechanism Spatial observatory Charged particles Secondary particle Field potential Electric potential Pulsars Signal-to-noise ratio Soft X radiation Curvature radiation Gamma radiation Synchrotron radiation
- Keyword (es)
- Aceleración partícula Angulo observación Emisión partícula Modelo Mecanismo radiación Observatorio espacial Partícula secundaria Potencial campo Radiación curvatura
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26224898
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
10.1088/0004-637X/748/2/84 
https://dx.doi.org/10.1088/0004-637X/748/2/84
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