3C 254: The alignment effect and unification schemes

被引:12
作者
Bremer, MN [1 ]
机构
[1] UNIV CAMBRIDGE,INST ASTRON,CAMBRIDGE CB3 0HA,ENGLAND
关键词
galaxies; clusters; general; cooling flows; quasars; emission lines; individual; 3C; 254;
D O I
10.1093/mnras/284.1.126
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
3C 254 is a radio-loud quasar at z=0.734. Optical line and continuum emission from the underlying galaxy is clearly extended and aligned with the radio axis; the object shows the so-called 'alignment effect' which is often seen in powerful radio galaxies, This is the dearest case yet of the continuum alignment effect in a radio-loud quasar, The object is one of the most lobe-dominated 3C quasars, the significance of the aligned emission in this source is discussed in terms of orientation-based unification schemes for radio-loud quasars and radio galaxies. 3C 254 is a very asymmetric radio source and it is shown that the radio structure on the side with the shortest nucleus-hotspot distance is interacting with the emission-line gas surrounding the quasar. It is also shown that the quasar is surrounded by an overdensity of faint objects, consistent with a cluster or group of galaxies around the object.
引用
收藏
页码:126 / 136
页数:11
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