Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003heba.conf..173m&link_type=abstract
High Energy Blazar Astronomy, ASP Conference Proceedings, Vol. 299, held 17-21 June 2002 at Tuorla Observatory, Piikkio, Finland
Astronomy and Astrophysics
Astronomy
1
Scientific paper
We have been carrying out multiwaveband observations in support of X-ray monitoring of blazars and the radio galaxy 3C 120 with the RXTE satellite. In 3C 120, we have observed four X-ray dips, each followed about 4 weeks later by ejections of superluminal radio knots down the jet. This behavior, of similar nature to that of the microquasar GRS 1915+105, is interpreted as infall of a section of the inner accretion disk causing energy to be ejected down the relativistic jet. The X-ray emission from the quasars PKS 1510-089, 3C 279, and 3C 273 shows pronounced variations on timescales as short as ˜ 1 day. Over a two-year period, X-ray flares in PKS 1510-089 peaked about 2 weeks after the maxima of radio outbursts. This ``reverse'' time lag can be explained by light-travel delays within the source. In 3C 279 the X-ray and optical variations were generally well correlated, with very small (perhaps zero) time delay. We conclude that the X-ray and optical emission from these quasars occurs near the radio core rather than close to the black hole.
Aller Margo F.
Balonek Thomas J.
Jorstad Svetlana G.
Marscher Alan P.
McHardy Ian M.
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