Intermediate BL Lac objects

被引:32
作者
Bondi, M
Marcha, MJM
Dallacasa, D
Stanghellini, C
机构
[1] Ist Radioastron, I-40129 Bologna, Italy
[2] Observ Astron Lisboa, CAAUL, P-1349018 Lisbon, Portugal
[3] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
[4] Ist Radioastron C da Renna Bassa, I-96017 Noto, Italy
关键词
galaxies : active; BL Lacertae objects : general; radio continuum : galaxies;
D O I
10.1046/j.1365-8711.2001.04519.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The 200-mJy sample, defined by Marcha et al., contains about 60 nearby, northern, flat-spectrum radio sources. In particular, the sample has proved effective at finding nearby radio-selected BL Lac objects with radio luminosities comparable to those of X-ray-selected objects, and low-luminosity flat-spectrum weak emission-line radio galaxies (WLRGs). The 200-mJy sample contains 23 BL Lac objects (including 6 BL Lac candidates) and 19 WLRGs. We will refer to these subsamples as the 200-mJy BL Lac sample and the 200-mJy WLRG sample, respectively. We have started a systematic analysis of the morphological pc-scale properties of the 200-mJy radio sources using VLBI observations. This paper presents VLBI observations at 5 and 1.6 GHz of 14 BL Lac objects and WLRGs selected from the 200-mJy sample. The pc-scale morphology of these objects is briefly discussed. We derive the radio beaming parameters of the 200-mJy BL Lac objects and WLRGs and compare them with those of other BL Lac samples and with a sample of FR I radio galaxies. The overall broad-band radio, optical and X-ray properties of the 200-mJy BL Lac sample are discussed and compared with those of other BL Lac samples, radio- and X-ray-selected. We find that the 200-mJy BL Lac objects fill the gap between HBL and LBL objects in the colour-colour plot, and have intermediate alpha (XOX) as expected in the spectral energy distribution unification scenario. Finally, we briefly discuss the role of the WLRGs.
引用
收藏
页码:1109 / 1123
页数:15
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