Open AccessIntermediate BL Lac objects
Author(s) -
Bondi M.,
Marchã M.J.M.,
Dallacasa D.,
Stanghellini C.
Publication year - 2001
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2001.04519.x
Subject(s) - physics , astrophysics , bl lac object , radio galaxy , very long baseline interferometry , astronomy , luminosity , galaxy , sample (material) , blazar , gamma ray , thermodynamics
The 200‐mJy sample, defined by Marchã 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 α XOX as expected in the spectral energy distribution unification scenario. Finally, we briefly discuss the role of the WLRGs.