J. Machalski et Wn. Brandt, THE RADIO, OPTICAL AND X-RAY-PROPERTIES OF THE RADIO-SOURCE-0927+352, Monthly Notices of the Royal Astronomical Society, 282(4), 1996, pp. 1305-1312
The radio structure of the source 0927 + 352 (87GB 092752.8 + 351642)
consists of a highly variable compact core and an extended diffuse hal
o, and comparison of its mas-scale and arcsec-scale structures suggest
s a twist of an internal jet and strong projection effects. Its optica
l counterpart varies by about 2 mag and shows no hint of emission line
s in its spectrum. A mean time-scale of radio variability of about 6(-
2)(+4) yr and a mean time delay between optical and radio 'events' of
about 4 yr are suggested by collected data. X-ray emission from 0927 352 was detected by the ROSAT satellite, and we report on its X-ray s
pectrum. 0927 + 352 is probably a rather slowly variable BL Lac, altho
ugh it could be a QSO with very weak emission lines.