光学剧变类星体
光学剧变类星体作为一种高变类星体,是耀变体中的一个子类型。光学剧变类星体一般由数个罕见的、明亮的电波星系组成,其发射的可见光的变化幅度在一日内可达到50%。其外部特征近似于蝎虎座BL型天体,但是该类星体往往具有更强的发射光谱以及更高的红移量。
单词 | OVV quasar |
释义 |
OVV quasar
中文百科
光学剧变类星体光学剧变类星体作为一种高变类星体,是耀变体中的一个子类型。光学剧变类星体一般由数个罕见的、明亮的电波星系组成,其发射的可见光的变化幅度在一日内可达到50%。其外部特征近似于蝎虎座BL型天体,但是该类星体往往具有更强的发射光谱以及更高的红移量。
英语百科
OVV quasar 光学剧变类星体![]() An optically violent variable quasar (often abbreviated as OVV quasar) is a type of highly variable quasar. It is a subtype of blazar that consists of a few rare, bright radio galaxies, whose visible light output can change by 50% in a day. OVV quasars have essentially become unified with highly polarized quasars (HPQ), core-dominated quasars (CDQ), and flat-spectrum radio quasars (FSRQ). Different terms are used but the term FSRQ is gaining popularity effectively making the other terms archaic. |
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