Abstract
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, albeit with modest radio fluxes (1-50 mJy). 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 (a ro = 0.30-0.51). The very bright X-ray-selected BL Lac objects like PKS 2155-304 and Markarian 501 have similar a ro 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.
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CITATION STYLE
Stocke, J. T., Morris, S. L., Gioia, I., Maccacaro, T., Schild, R. E., & Wolter, A. (1990). No evidence for radio-quiet BL Lacertae objects. The Astrophysical Journal, 348, 141. https://doi.org/10.1086/168221
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