COMPTEL observations of the gamma-ray blazar PKS 1622-297 | |
Zhang S(张澍); Zhang, S; Collmar, W; Bennett, K; Bloemen, H; Hermsen, W; McConnell, M; Reimer, O; Schonfelder, V; Wagner, SJ | |
刊名 | ASTRONOMY & ASTROPHYSICS |
2002 | |
卷号 | 386期号:3页码:843-853 |
关键词 | gamma rays : observations galaxies : active galaxies : quasars : individual : PKS 1622-297 |
通讯作者 | Max Planck Inst Extraterr Phys, D-85740 Garching, Germany ; SRON, Natl Inst Space Res, NL-3584 CA Utrecht, Netherlands ; Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA ; European Space Agcy, Dept Space Sci, Div Astrophys, ESTEC, NL-2200 AG Noordwijk, Netherlands ; NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA ; Inst High Energy Phys, Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China ; Landessternwarte Heidelberg, D-69117 Heidelberg, Germany |
英文摘要 | We report results of observations and analyses on the gamma-ray blazar PKS 1622-297, with emphasis on the COMPTEL data (0.75-30 MeV) collected between April 1991 and November 1997. PKS 1622-297 was detected as a source of gamma-rays by the EGRET experiment aboard CGRO in 1995 during a gamma-ray outburst at energies above 100 MeV lasting for five weeks. In this time period the blazar was significantly (similar to 5.9 sigma) detected by COMPTEL at 10{30 MeV. At lower COMPTEL energies the detection is marginal, resulting in a hard MeV spectrum. The combined COMPTEL/EGRET energy spectrum shows a break at MeV energies. The broad-band spectrum (radio {-gamma-rays) shows that the gamma-ray emission dominates the overall power output. On top of the 5-week gamma-ray outburst, EGRET detected a huge are lasting for >1 day. Enhanced MeV emission (10-30 MeV) is found near the time of this are, suggesting a possible time delay with respect to the emission above 100 MeV. Outside the 5-week flaring period in 1995, we do not detect MeV emission from PKS 1622-297. |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
原文出处 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000175269800009 |
内容类型 | 期刊论文 |
源URL | [http://ir.ihep.ac.cn/handle/311005/238591] |
专题 | 高能物理研究所_粒子天体物理中心 |
作者单位 | 中国科学院高能物理研究所 |
推荐引用方式 GB/T 7714 | Zhang S,Zhang, S,Collmar, W,et al. COMPTEL observations of the gamma-ray blazar PKS 1622-297[J]. ASTRONOMY & ASTROPHYSICS,2002,386(3):843-853. |
APA | 张澍.,Zhang, S.,Collmar, W.,Bennett, K.,Bloemen, H.,...&Williams, OR.(2002).COMPTEL observations of the gamma-ray blazar PKS 1622-297.ASTRONOMY & ASTROPHYSICS,386(3),843-853. |
MLA | 张澍,et al."COMPTEL observations of the gamma-ray blazar PKS 1622-297".ASTRONOMY & ASTROPHYSICS 386.3(2002):843-853. |
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