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Advances in Space Research

Volumn 27, Issue 4, 2001, Pages 653-658

Vela as the most likely source for the primary electrons in Tev region

(4) Kobayashi, T a Nishimura, J b Komori, Y c Yoshida, K d

a AOYAMA GAKUIN UNIVERSITY (Japan)

b JAPAN AEROSPACE EXPLORATION AGENCY (Japan)

c Department of Internal Medicine (Japan)

d KANAGAWA UNIVERSITY (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

COSMIC RAYS; ELECTRONS; ENERGY DISSIPATION; GALAXIES; SOLAR SYSTEM; SYNCHROTRONS;

SUPERNOVA REMNANTS (SNRS);

HIGH ENERGY PHYSICS;

COSMIC RAY; ELECTRON;

EID: 0034925324 PISSN: 02731177 EISSN: None Source Type: Journal
DOI: 10.1016/S0273-1177(01)00106-5 Document Type: Article

Times cited : (7)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.