Published March 1, 1986
| Version v1
Journal article
PKS 2005-489; a very bright BL Lac object in a nearby galaxy
- 1. Royal Greenwich Observatory, Hailsham (UK)
- 2. European Southern Observatory, Garching (Germany, F.R.)
- 3. Leicester Univ. (UK). Dept. of Physics
- 4. European Space Agency, Madrid (Spain). Villafranca Satellite Tracking Station
Description
The galaxy identified with the flat-spectrum radio source PKS2005-489 has a bright and variable stellar nucleus with a brightest observed V magnitude of approx. 13. Reported here are radio, optical, UV and X-ray observations which indicate variability and power-law continua in each of these wavebands, leading to the conclusion that PKS2005-489 is one of the brightest BL Lac objects known. The ultraviolet data show unusually strong absorption lines formed in the interstellar medium of our Galaxy, but no obvious features due to the host galaxy. The X-ray output in the range 0.04-6keV is far in excess of a simple power-law extrapolation from lower frequencies. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 219
- Journal Issue
- 1
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 23P-29P
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 17046248
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- ABSORPTION SPECTRA; BL LACERTAE OBJECTS; BRIGHTNESS; COSMIC RADIO SOURCES; EMISSION SPECTRA; EXPERIMENTAL DATA; GALAXIES; GALAXY NUCLEI; ULTRAVIOLET SPECTRA; VARIATIONS; VISIBLE SPECTRA
- Descriptors DEC
- COSMIC RAY SOURCES; COSMIC X-RAY SOURCES; DATA; INFORMATION; NUMERICAL DATA; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SPECTRA