Interrelation between radio and X-ray signatures of drifting subpulses in pulsars
- Author
- GIL, J1 2 ; MELIKIDZE, G1 3 ; ZHANG, B2
[1] Institute of Astronomy, University of Zielona Góra, Lubuska 2, 65-265 Zielona Góra, Poland
[2] Department of Physics, University of Nevada, Las Vegas, United States
[3] Abastumani Astrophysical Observatory, Al. Kazbegi ave. 2a, 0160 Tbilisi, Georgia - Source
Astronomy and astrophysics (Berlin. Print). 2006, Vol 457, Num 1 ; L5-L8 ; ref : 22 ref
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- X-ray: stars pulsars: general radiation mechanism: thermal stars: neutron
- Keyword (fr)
- Corrélation Etoile neutron Luminosité Modèle Mécanisme rayonnement Plasma Positon Pulsar Périodicité Rayonnement thermique Vitesse chauffage
- Keyword (en)
- Correlations Neutron stars Luminosity Models Radiation mechanism Plasma Positrons Pulsars Periodicity Thermal radiation Heat rate
- Keyword (es)
- Modelo Mecanismo radiación Periodicidad
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18108575
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
10.1051/0004-6361:20065228 
https://dx.doi.org/10.1051/0004-6361:20065228
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