X-Ray Variability in the Jet and Core of M87

Details X-Ray Variability in the Jet and Core of M87 X-Ray Variability in the Jet and Core of M87

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1264h&link_type=abstract

Chandra Proposal ID #04700315

Mathematics

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Chandra Proposal Id #04700315

Scientific paper

M87 is the nearest galaxy with a bright radio / optical / X-ray jet, and affords an unparalleled opportunity to study extragalactic jet phenomena at high resolution. We propose the second phase of a long-term variability study of the core and jet of M87 with 8 ACIS observations at intervals of 1.3 months. We will correlate X-ray brightness variations in both time and place with morphological features (shocks within knots) and structural changes (emergence of new superluminal features) seen in our high resolution radio / optical studies of the 20" jet. Our ultimate goal is to learn what processes and phyical conditions are responsible for producing X-rays in AGN jets.

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