Very high energy gamma rays from the vela pulsar direction

Astrophysical Journal

Volumn 487, Issue 1 PART II, 1997, Pages

  Yoshikoshi, T ^a,b   Kifune, T ^b   Dazeley, S A ^c   Edwards, P G ^c,d   Hara, T ^e   Hayami, Y ^a   Kakimoto, F ^a   Konishi, T ^f   Masaike, A ^g   Matsubara, Y ^h   Matsuoka, T ^h   Mizumoto, Y ⁱ   Mori, M ^j   Muraishi, H ^k   Muraki, Y ^h   Naito, T ^b   Nishijima, K ^l   Oda, S ^f   Ogio, S ^a   Ohsaki, T ^a   Patterson, J R ^c   Roberts, M D ^b   Rowell, G P ^c   Sako, T ^h   Sakurazawa, K ^a   Susukita, R ^g,m   Suzuki, A ^f   Tamura, T ⁿ   Tanimori, T ^a   Thornton, G J ^b,c   Yanagita, S ^k   Yoshida, T ^k   more..

^a TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c UNIVERSITY OF ADELAIDE   (Australia)

^d JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^e YAMANASHI GAKUIN UNIVERSITY   (Japan)

^f KOBE UNIVERSITY   (Japan)

^g KYOTO UNIVERSITY   (Japan)

^h NAGOYA UNIVERSITY   (Japan)

ⁱ NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^j MIYAGI UNIVERSITY OF EDUCATION   (Japan)

^k IBARAKI UNIVERSITY   (Japan)

^l TOKAI UNIVERSITY   (Japan)

^m INST OF PHYS AND CHEMICAL RESEARCH   (Japan)

ⁿ KANAGAWA UNIVERSITY   (Japan)

more..

Author keywords

Gamma rays: observations; ISM: individual (Vela supernova remnant); ISM: magnetic fields; Pulsars: individual (Vela pulsar); Supernova remnants

Indexed keywords

EID: 21944433405     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310874     Document Type: Article

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