Abstract
The radio structure of the source 0927 + 352 (87GB 092752.8 + 351642) consists of a highly variable compact core and an extended diffuse halo, and comparison of its mas-scale and arcsec-scale structures suggests a twist of an internal jet and strong projection effects. Its optical counterpart varies by about 2 mag and shows no hint of emission lines 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 spectrum. 0927 + 352 is probably a rather slowly variable BL Lac, although it could be a QSO with very weak emission lines.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1305-1312 |
| Number of pages | 8 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 282 |
| Issue number | 4 |
| DOIs | |
| State | Published - 1996 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science