No evidence for radio-quiet BL Lacertae objects
Creators
- 1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)
- 2. Mount Wilson and Las Campanas Observatories, Pasadena, CA (USA)
- 3. Colorado Univ., Boulder (USA)
Description
Using a large, flux-limited sample of faint X-ray sources, a search has been conducted for radio-quiet BL Lacertae objects. None has been found. Thirty-two X-ray-selected BL Lac objects and BL Lac candidates have been found within the sources of the Einstein Medium Sensitivity Survey (EMSS). Thirty-one of these have been observed with the VLA and all have been detected at 5 GHz. While the optical magnitudes of the EMSS BL Lac objects range from 17 to 20.8, their radio-to-optical spectral indices occupy a very small range. The very bright X-ray-selected BL Lac objects like PKS 2155-304 and Markarian 501 have similar range values. Therefore, unlike the clear dichotomy between radio-loud quasars and radio-quiet QSOs, there is no evidence for two populations of Lacertids distinguished by radio loudness. 43 refs
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 348
- Series
- Astrophys. J.
- Journal Page Range
- 141-146
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21055610
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BL LACERTAE OBJECTS; COSMIC RADIO SOURCES; COSMIC X-RAY SOURCES; MILKY WAY; ORGANIZING; QUASARS; RADIOWAVE RADIATION
- Descriptors DEC
- COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; GALAXIES; RADIATIONS