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Co-ordinated VSOP and Chandra Observations of 0836+710

Published online by Cambridge University Press:  13 May 2016

D.W. Murphy ,
R.A. Preston ,
G.B. Piner ,
M.L. Lister ,
H.L. Marshall  and
P.G. Edwards
D.W. Murphy
Affiliation:
JPL, MS 238-332, 4800 Oak Grove Drive, Pasadena, CA 91101, USA
R.A. Preston
Affiliation:
JPL, MS 238-332, 4800 Oak Grove Drive, Pasadena, CA 91101, USA
G.B. Piner
Affiliation:
JPL, MS 238-332, 4800 Oak Grove Drive, Pasadena, CA 91101, USA
M.L. Lister
Affiliation:
JPL, MS 238-332, 4800 Oak Grove Drive, Pasadena, CA 91101, USA
H.L. Marshall
Affiliation:
Center for Space Research, MIT, Cambridge, MA 02139, USA
P.G. Edwards
Affiliation:
ISAS, Yoshinodai 3-1-1, Sagamihara, Kanagawa 229-8510, Japan

Abstract

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We briefly describe the radio observations that form part of co-ordinated Chandra, HALCA+VLBA, and VLBA-only observations of the superluminal gamma-ray loud quasar 0836+710. The radio observations were at 6 frequencies (1.6, 5, 8, 15, 22, and 43 GHz) with the two lowest frequency observations being undertaken with the VLBA co-observing with the HALCA spacecraft (the space element of the Japanese VSOP mission). Combining the radio and X-ray data will allow constraints to be placed on the jet Doppler factor.

Type
The Inner Regions of Galaxies
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 126 - 127
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Murphy, D. W. et al. 2000, in Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W., (Sagamihara: ISAS) 219.Google Scholar