A Search for Low‐Luminosity BL Lacertae Objects

Abstract

Many properties of BL have become explicable in terms of the relativistic beaming hypothesis whereby BL are FR-1 radio galaxies viewed nearly along the jet axis. However, a possible problem with this model is that a transition population between beamed BL and unbeamed FR-1s has not been detected. A transition population of low-luminosity BL Lacs was predicted to exist in abundance in X-ray-selected samples such as the Einstein Extended Medium Sensitivity Survey (EMSS) by Browne & Marcha. However, these BL may have been misidentified as clusters of galaxies. We have conducted a search for such objects in the EMSS with the ROSAT HRI; and here we present ROSAT HRI images, optical spectra and VLA radio maps for a small number of BL which were previously misidentified in the EMSS catalog as clusters of galaxies. While these objects are slightly lower in luminosity than other EMSS BL Lacs, their properties are too similar to the other BL in the EMSS sample to bridge the gap between BL and FR-1 radio galaxies. Also, the number of new BL found are too few to alter significantly the X-ray luminosity function or value for the X-ray-selected EMSS BL Lac sample. Thus, these observations do not explain fully the discrepancy between the X-ray and radio-selected BL Lac samples.