NO EVIDENCE FOR RADIO-QUIET BL LACERTAE OBJECTS

被引:97
作者
STOCKE, JT
MORRIS, SL
GIOIA, I
MACCACARO, T
SCHILD, RE
WOLTER, A
机构
[1] CARNEGIE INST WASHINGTON,THE OBSERV,WASHINGTON,DC 20005
[2] HARVARD SMITHSONIAN CTR ASTROPHYS,CAMBRIDGE,MA 02138
关键词
BL Lacertae objects; Radio sources: galaxies;
D O I
10.1086/168221
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 (αro = 0.30-0.51). The very bright X-ray-selected BL Lac objects like PKS 2155-304 and Markarian 501 have similar αro 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.
引用
收藏
页码:141 / 146
页数:6
相关论文
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