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VLBI Observations of Southern EGRET Identifications

Published online by Cambridge University Press:  25 May 2016

J.E.J. Lovell ,
S.J. Tingay ,
P.G. Edwards ,
D.L. Jauncey  and
R.A. Preston
J.E.J. Lovell
Affiliation:
1 Department of Physics, University of Tasmania - Hobart, 7001, Australia
S.J. Tingay
Affiliation:
2 Mount Stromlo and Siding Spring Observatories - ACT 2611, Australia
P.G. Edwards
Affiliation:
3 Institute of Space and Astronautical Science - Sagamihara, Kanagawa 229, Japan
D.L. Jauncey
Affiliation:
4 Australia Telescope National Facility - Epping, 2121, Australia
R.A. Preston
Affiliation:
5 Jet Propulsion Laboratory - Pasadena, 91109, USA

Extract

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We present high resolution VLBI images of three southern radio sources: PKS 0208–512, PKS 0521–365 and PKS 0537–441. These sources have been identified as > 100 MeV gamma-ray sources with the Energetic Gamma-Ray Telescope (EGRET) on board the Compton Gamma-Ray Observatory (Thompson et al. 1995). These are the first results in a continuing program of VLBI observations of southern EGRET identifications with the Southern Hemisphere VLBI Experiment (SHEVE) array of telescopes (Jauncey et al., 1994).

Type
Properties of Radio Sources
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 19 - 20
Copyright
Copyright © Kluwer 1996 

References

Jauncey, D.L. et al.: 1994 “Very High Angular Resolution Imaging” , Roberston, J.G. and Tango, W.J. (eds), p 131–134 Google Scholar
Thompson, D.J. et al.: 1995, Astrophys. J., Suppl. Ser., in press Google Scholar