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Multiband VLBI observations of CTA 102

Rantakyrö, Fredrik T. (author)
Dept. of Astronomy and Astrophysics, University of Gothenburg, S-412 96 Gothenburg, Sweden
Bååth, Lars B. (author)
Onsala Space Observatory, S-439 92 Onsala, Sweden
Dallacasa, Daniele (author)
Istituto di RadioAstronomia, CNR, Via Gobetti 101, I-40129, Bologna, Italy
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Jones, Dayton L. (author)
Jet Propulsion Laboratory, Pasadena, CA 91109, United States
Wehrle, Ann E. (author)
Infrared Proc. and Analysis Center, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91125, United States
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Dept of Astronomy and Astrophysics, University of Gothenburg, S-412 96 Gothenburg, Sweden Onsala Space Observatory, S-439 92 Onsala, Sweden (creator_code:org_t)
EDP Sciences, 1996
1996
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 310:1, s. 66-74
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The source CTA102, known to exhibit low frequency variability, has been observed at six epochs (three at λ32cm, two at λ18cm, and one at λ1.3cm) with intercontinental VLBI arrays. On the basis of the changes observed in the structure, we believe that the flux density variations at these wavelengths are due to intrinsic processes and not due to interstellar scintillation. This source exhibits behaviour suggestive of being expanding with a very high apparent transverse velocity.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

Galaxies
Quasars
CTA 102
Physics
Fysik

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art (subject category)

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