X-ray spectral analyses of the M87 jet

Details X-ray spectral analyses of the M87 jet X-ray spectral analyses of the M87 jet

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.150m&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Computer Science

Agn Jets

Scientific paper

We present X-ray spectral analyses of the jet in the giant radiogalaxy M87. We derive spectral parameters of the X-ray emission between the radio knots from the various long observations in the Chandra archive. In addition we use the 60 monitoring observations(5ks each, spanning the last 7 years) to evaluate the X-ray spectral variability of the three brightest knots, HST-1, D, and A. This project is one component of a broader investigation of the spectral energy distribution for all parts of the entire jet. The work at SAO was supported by NASA grants GO8-9116X and GO9-0108X.

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