ROSAT HRI observation of the supernova remnant Kes 32 and the nearby radio pulsar PSR B1610-50
著者
和文:
Brinkmann, W.,
河合 誠之,
Scheingraber, H.,
Tamura, K.,
Becker, W..
英文:
Brinkmann, W.,
Kawai, N.,
Scheingraber, H.,
Tamura, K.,
Becker, W..
言語
English
掲載誌/書名
和文:
英文:
Astronomy and Astrophysics
巻, 号, ページ
Vol. 346
pp. 599-603
出版年月
1999年6月
出版者
和文:
英文:
会議名称
和文:
英文:
開催地
和文:
英文:
アブストラクト
We present the results of a deep ROSAT HRI observation of the supernova remnant Kes 32 and the possibly associated pulsar PSR B1610-50. The supernova remnant shows strongly energy dependent complex structures in a comparison with the ASCA GIS and ROSAT PSPC data with low foreground absorption (N_H ~ 5*E(21) cm(-2) ). The pulsar is not seen in the HRI image indicating a high absorbing column density (N_H >~ 5*E(22) cm(-2) ) along the line of sight, making the physical connection between Kes 32 and PSR B1610-50 unlikely. The elongated structure south of the pulsar, interpreted as a pulsar jet, might be an unrelated foreground emission.
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