X-RAY EVIDENCE THAT 3C273 IS IN THE VIRGO-CLUSTER

被引：3

作者：

ARP, HC

机构：

[1] Max-Planck-Institut für Astrophysik

来源：

PHYSICS LETTERS A | 1995年 / 203卷 / 04期

关键词：

D O I：

10.1016/0375-9601(95)00343-2

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

was shown that the giant radio galaxy 3C274 (M87) and the brightest quasar, 3C273, were almost exactly aligned across the central galaxy in the Virgo Cluster (M49). During the ensuing years additional evidence has accumulated that 3C273 (redshift, z = 0.158) is a member of the Virgo Cluster (z = 0.003). Now low surface brightness X-ray features recorded in the ROSAT all sky survey reveal that both M87 and 3C273 are physically connected back to M49.

引用

页码：161 / 164

页数：4

共 50 条

[1] X-RAY SPECTRAL VARIABILITY OF 3C273
TURNER, MJL
COURVOISIER, T
STAUBERT, R
MOLTENI, D
TRUMPER, J
SPACE SCIENCE REVIEWS, 1985, 40 (3-4) : 623 - 626
[2] 4 YEARS OF RADIO TO X-RAY OBSERVATIONS OF 3C273
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ROBSON, EI
BLECHA, A
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IAU SYMPOSIA, 1989, (134): : 112 - 113
[3] Soft X-ray variability of the bright quasar 3C273
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[4] 4 YEARS OF RADIO TO X-RAY OBSERVATIONS OF 3C273
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[5] Soft X-ray variability of the bright quasar 3C273
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[6] CORRELATED X-RAY AND MILLIMETER VARIABILITY OF THE BLAZAR 3C273
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[7] THE X-RAY-EMISSION OF 3C273
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[8] X-RAY OBSERVATIONS OF VIRGO CLUSTER, NGC-5128, AND 3C-273 FROM UHURU SATELLITE
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[9] Simultaneous X-ray and infrared variability in the quasar 3C273 - II. Confirmation of the correlation and X-ray lag
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[10] RESULTS OF LIMITATIONS ON THE X-RAY SOURCE SIZE ON GAMMA-RADIATION FROM 3C273
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ASTRONOMY & ASTROPHYSICS, 1979, 71 (03) : L19 - L21

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