Spectral energy distributions of five FR I radio galaxies

被引：6

作者：

Capetti, A ^{[1
]}

Trussoni, E

Celotti, A

Feretti, L

Chiaberge, A

机构：

[1] Osserv Astron Torino, I-10025 Pino Torinese, Italy

[2] SISSA, I-34014 Trieste, Italy

[3] CNR, Ist Radioastron, I-40126 Bologna, Italy

来源：

NEW ASTRONOMY REVIEWS | 2002年 / 46卷 / 2-7期

关键词：

BL lacertae objects : general; galaxies : active; radiation mechanisms : non-thermal; radio continuum : galaxies;

D O I：

10.1016/S1387-6473(01)00203-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We discuss the multi-wavelength properties of the radio galaxies 3C 31, 3C 264, 3C 270, 3C 465 and NGC 7052. The data have been deduced from observations with the VLBI/VLA arrays, HST and ROSAT. The SED of these sources, when compared with that of BL Lacs shows that beaming effects are important, but are not enough-in the simplest scenario-to explain the different properties of these two classes of objects. No relevant obscuration from inner tori seems to occur. (C) 2002 Published by Elsevier Science B.V.

引用

收藏

页码：335 / 337

页数：3

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