NEWLY BORN PULSARS AS SOURCES OF ULTRAHIGH ENERGY COSMIC RAYS
- Author
- KE FANG1 ; KOTERA, Kumiko1 2 ; OLINTO, Angela V1
[1] Department of Astronomy & Astrophysics, Kavli Institute for Cosmological Physics, The University of Chicago, Chicago, IL 60637, United States
[2] Theoretical Astrophysics, California Institute of Technology, 1200 E California Blvd., M/C 350-17, Pasadena, CA 91125, United States - Source
The Astrophysical journal. 2012, Vol 750, Num 2 ; 118.1-118.16 ; 1 ; ref : 3/4 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
- astroparticle physics cosmic rays pulsars: general supernovae: general
- Keyword (fr)
- Champ dipolaire Dipôle magnétique Effondrement Elément lourd Elément léger Noyau lourd Nucléon Proton Pulsar milliseconde Rayonnement cosmique Supernova
- Keyword (en)
- Dipole field Magnetic dipoles Collapse Heavy element Light element Heavy nuclei Nucleons Protons Millisecond pulsar Cosmic radiation Supernovae
- Keyword (es)
- Campo dipolar Desmoronamiento Elemento pesado Elemento ligero Pulsar milisegundo
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26195474
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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