Radio morphology and parent population of X-ray selected BL Lacertae objects

Details Radio morphology and parent population of X-ray selected BL Lacertae objects Radio morphology and parent population of X-ray selected BL Lacertae objects

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....106..875l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 106, no. 3, p. 875-898.

Astronomy and Astrophysics

Astronomy

61

Bl Lacertae Objects, Radio Astronomy, Galactic Clusters, Heao 1, Radio Galaxies, Radio Jets (Astronomy), Sky Surveys (Astronomy), Spaceborne Astronomy, Very Large Array (Vla)

Scientific paper

High-dynamic range (typically 1700:1) radio maps of 15 X-ray BL Lac (XBL) objects from the HEAO-1 Large Area Sky Survey are presented. Morphological characteristics of these sources are compared with Fanaroff-Riley (FR) class I radio galaxies in the context of unified schemes, with reference to one-sided kiloparsec-scale emission. Evidence that cluster membership of XBLs is significantly higher than previously thought is also presented. It is shown that the extended radio powers, X-ray emission, core-to-lobe ratios, and linear sizes of the radio selected BL Lac (RBL) and XBL populations are consistent with an FR I radio galaxy parent population. A source list and VLA observing log and map parameters are provided.

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