Published January 1990 | Version v1
Journal article

No evidence for radio-quiet BL Lacertae objects

  • 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