ANALYTIC SOLUTION FOR SELF-REGULATED COLLECTIVE ESCAPE OF COSMIC RAYS FROM THEIR ACCELERATION SITES.

Malkov, M A; Diamond, P H; Sagdeev, R Z; Aharonian, F A; Moskalenko, I V

Malkov, M A; Diamond, P H; Sagdeev, R Z; Aharonian, F A; Moskalenko, I V.

Affiliation

Malkov MA; CASS and Department of Physics, University of California, San Diego, La Jolla, CA 92093, USA.
Diamond PH; Kavli Institute for Particle Astrophysics and Cosmology, Stanford, CA 94305, USA.
Sagdeev RZ; CASS and Department of Physics, University of California, San Diego, La Jolla, CA 92093, USA.
Aharonian FA; Also at WCI Center for Fusion Theory, NFRI, Korea.
Moskalenko IV; University of Maryland, College Park, MD 20742-3280, USA.

Astrophys J ; 768(1)2013 May 01.

Article de En | MEDLINE | ID: mdl-34646037

Mots clés

ISM: individual objects (W44, W51C, IC 443, W28); ISM: supernova remnants; acceleration of particles; cosmic rays; diffusion

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Texte intégral: 1 Collection: 01-internacional Base de données: MEDLINE Langue: En Journal: Astrophys J Année: 2013 Type de document: Article Pays d'affiliation: États-Unis d'Amérique Pays de publication: États-Unis d'Amérique

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