Radio Objects with Continuous Optical Spectra, (abbr. ROCOS, also referred to as ROCOSes) is a group of about 80 astrophysical objects characterized by optical spectra anomalously devoid of emission or absorption features, which makes it impossible to determine their distances and locations in relation to our galaxy.[1][2][3] They are considered to be a subclass of blazars, and are similar in their spectral characteristics to DC-dwarfs and single stellar-mass black holes.[4]

Discovery and study

The 6-meter optical telescope at the Special Astrophysical Observatory of the Russian Academy of Science used for studying ROCOSes

Radio Objects with Continuous Optical Spectra, or ROCOSes, were discovered in the 1970s.[1] Among the discoverers was a group of Soviet astrophysicists, who studied them at the Crimean Astrophysical Observatory and the Special Astrophysical Observatory of the Russian Academy of Science, using the former's 2.6-meter optical telescope and the latter's 6-meter optical telescope (BTA-6), along with a 1000-channel photon counter and photometers.[1][2][3] The group published their findings in a series of articles in the Russian scientific journals Astronomy Letters and Astronomy Reports.[1][2]

Criteria

An astronomical radio object is classified as a ROCOS if it possesses (a) an optical image with stellar appearance, which is identified with a radio source, and (b) no emission or absorption features in its optical spectrum, except for those due to galactic interstellar medium, with a signal-to-noise ratio at the level of those observable for quasar candidates.[1] About 8% of the known astronomical radio objects satisfy these two criteria and are considered ROCOSes.[2][3]

Properties

The absence of distinct emission or absorption lines in the ROCOSes' spectra makes them very similar in this regard to highly polarized quasars (HPQ), BL Lac objects, and single stellar-mass black holes.[2][4] The absence of optical spectral features also makes it impossible to use red shift for determining their distances or even ascertaining if they are located within or outside our galaxy.[2]

References

  1. 1 2 3 4 5 Beskin, G. M.; Efimov, Y. S.; Neizvestni, S. I.; Pustilnik, S. A.; Shakhovskoi, N. M. (1981). "Radio Objects with a Continuous Optical Spectrum - Part One - an Optical Polarization Survey". Soviet Astronomy Letters. American Institute of Physics. 7: 391. Bibcode:1981SvAL....7..391B. Retrieved 26 May 2012.
  2. 1 2 3 4 5 6 Lipovetskii, V. A.; Pustilnik, L. A.; Pustilnik, S. A.; Shapovalova, A. I. (Nov 1989). "Radio Objects with Continuous Optical Spectra - Search for Spectral Features Using the 6-METER Telescope". Soviet Astronomy. American Institute of Physics. 33 (6): 585. Bibcode:1989SvA....33..585L. Retrieved 26 May 2012.
  3. 1 2 3 Lipovetskii, V. A.; Pustil'nik, L. A.; Pustil'nik, S. A.; Shapovalova, A. I. (Nov–Dec 1989). "A study of radio objects with continuous optical spectra - Search for spectral features with the six-meter telescope". Astronomicheskii Zhurnal. The Smithsonian/NASA Astrophysics Data System. 66: 1132–1141. Bibcode:1989AZh....66.1132L. ISSN 0004-6299.
  4. 1 2 Matt, Giorgio (2007). Black Holes from Stars to Galaxies, Across the Range of Masses: Proceedings of the 238th Symposium of the International Astronomical Union, Held in Prague, Czech Republic August 21-25, 2006. Cambridge University Press. p. 160. ISBN 9780521863476. Retrieved 26 May 2012.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.