Published September 1982 | Version v1
Journal article

Optical absorption lines in the high redshift BL Lac object 0215 + 015

  • 1. Science Research Council, Chilton (UK). Rutherford and Appleton Labs.
  • 2. Anglo-Australian Observatory, Epping (Australia)
  • 3. Sydney Univ. (Australia). School of Physics
  • 4. Royal Greenwich Observatory, Hailsham (UK)

Description

We present results from our study of 0215 + 015 (PKS 0215 + 015), the highest redshift and most luminous BL Lac object so far detected. Optical continuum measurements show that the object had brightened to 15.2 mag on 1980 September 10, thus confirming an overall variability range of more than 4 mag. Variations on a time-scale of =< 2 months may also be present. A review of the published radio data indicates that 0215 + 015 has a core-halo or multi-component structure, similar to that found for the BL Lac 0735 + 178. Four absorption redshift systems occur with zsub(a) = 1.254, 1.345, 1.549 and 1.649. The zsub(a) = 1.345 system exhibits a rich, mixed-ionization spectrum whilst the other three are predominantly C IV systems. All four show complex structure when observed at high resolution. Possible origins of the absorption systems are discussed. Column densities of the zsub(a) = 1.345 system are very similar to those found for our Galaxy in sight-lines towards the Magellanic Clouds, and an origin in an intervening galaxy seems almost certain for this system. The velocity structure and line-widths of the 1.649 system are less plausibly due to intervening galaxies, but are consistent with the intrinsic absorption model of Dyson, Falle and Perry (1980). (author)

Additional details

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
200
Journal Issue
3
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
1091-1111
ISSN
0035-8711