Constraint of Non-Thermal X-Ray Emission from the On-Going Merger Cluster Abell 3376 with Suzaku

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Department ofPhysical Science, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan ^{[1
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来源：

Publ. Astron. Soc. Jpn. | 2009年 / SUPPL. 1卷 / S377-S386期

关键词：

Galaxies;

D O I：

10.1093/pasj/61.sp1.s377

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引用

共 6 条

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ASTRONOMY & ASTROPHYSICS, 2021, 654
[2] X-ray emission from the galaxies in Abell 2634
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 293 (04) : 489 - 496
[3] X-ray emission from the Fornax cluster
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ASTROPHYSICAL JOURNAL, 1997, 482 (01): : 143 - 155
[4] THE X-RAY LUMINOSITY FUNCTIONS OF ABELL CLUSTERS FROM THE EINSTEIN CLUSTER SURVEY
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ASTROPHYSICAL JOURNAL, 1994, 422 (01): : 37 - 45
[5] X-ray emission from the cluster around E1821+643
Saxton, RD
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Turner, MJL
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Stewart, GC
Kii, T
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 289 (01) : 196 - 202
[6] Analysis and interpretation of hard X-ray emission from the bullet cluster (1ES 0657-558), the most distant cluster of galaxies observed by RXTE
Petrosian, Vahe
Madejski, Greg
Luli, Kevin
ASTROPHYSICAL JOURNAL, 2006, 652 (02): : 948 - 954