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The milliarcsecond scale structure of low frequency variable sources

Romney, J. (author)
Max-Planck-Institut für Radioastronomie, Bonn, Germany
Padrielli, L. (author)
CNR, Istituto di Radioastronomia, Bologna, Italy
Bartel, N. (author)
Max-Planck-Institut für Radioastronomie, Bonn, Germany & Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
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Weiler, K.W. (author)
Max-Planck-Institut für Radioastronomie, Bonn, Germany & Division of Astronomical Sciences, National Science Foundation, Washington, DC, USA
Ficarra, A. (author)
CNR, Istituto di Radioastronomia, Bologna, Italy
Mantovani, F. (author)
CNR, Istituto di Radioastronomia, Bologna, Italy
Bååth, L.B. 1948- (author)
Onsala Space Observatory, Chalmers University of Technology, Gothenburg, Sweden
Kogan, L. (author)
Institute for Space Research, Academy of Sciences, Moscow, USSR
Matveenko, L. (author)
Institute for Space Research, Academy of Sciences, Moscow, USSR
Moiseev, I.G. (author)
Crimea Astrophysical Observatory, Academy of Sciences, Moscow, USSR
Nicholson, G. (author)
National Institute for Telecommunications Research, Johannesburg, South Africa
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 (creator_code:org_t)
Les Ulis : EDP Sciences, 1984
1984
English.
In: Astronomy and Astrophysics. - Les Ulis : EDP Sciences. - 0004-6361 .- 1432-0746. ; 135:2, s. 289-299
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • VLBI observations were performed of 21 radio sources which exhibit low frequency variability. The integrated flux densities, variability indices at 0.4 GHz, optical magnitudes, redshifts, spectral indices at 0.4 GHz, and flux intensities with respect to a reference energy flux are provided. The VLBI data were synthesized from observatories located on different continents around the world. All structures were emitted from compact sources with sizes confined to milliarcsc scales. Nearly half displayed core-jet morphologies, while 28 percent had complex structures and 14 percent had either simple structures or were not resolvable. Further observations are proceeding at 400 mHz to confirm the presence of synchrotron electrons and magnetic fields ejected at relativistic speeds along the line of sight, which has the appearance of superluminal velocities.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

low frequency variables
interferometry
VLBI
radio sources: general

Publication and Content Type

ref (subject category)
art (subject category)

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