Analysis of multicolor observations of 3C 66A in 1993-1998

被引：3

作者：

Hagen-Thorn V.A. ^{[1
]}

Hagen-Thorn A.V. ^{[1
]}

Jorstad S.G. ^{[1
,2
]}

Takalo L.O. ^{[3
]}

Sillanpää A. ^{[3
]}

Pursimo T. ^{[3
]}

Boltwood P. ^{[4
]}

机构：

[1] Saint Petersburg State University,

[2] Saint Petersburg State University,undefined

[3] Boston University,undefined

[4] University of Turku,undefined

[5] Boltwood Observatory,undefined

来源：

Astrophysics | 2001年 / 44卷 / 3期

关键词：

Energy Distribution; Variable Source; Synchrotron Nature; Multicolor Observation;

D O I：

10.1023/A:1012809409416

中图分类号：

学科分类号：

摘要：

The results of multicolor observations of the blazar 3C 66A, obtained in the course of the project OJ-94, are analyzed. It is established that the energy distribution of the variable source in the optical and IR ranges can be represented, on the average, by a power law: Fv ∝ v-0.92. Since the blazar's emission is strongly polarized, there is no doubt of the synchrotron nature of the variable source responsible for the blazar's activity. ©2001 Plenum Publishing Corporation.

引用

页码：283 / 291

页数：8

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