Large scale radio/X-ray jets in microquasars

Details Large scale radio/X-ray jets in microquasars Large scale radio/X-ray jets in microquasars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1258c&link_type=abstract

ATNF proposal C1199, Semester: April, 2008

Computer Science

Galactic, Atca

Scientific paper

The discovery with ATCA of large scale radio lobes around the microquasar XTE J1550-564 has led to the discovery with Chandra (for the first time) of moving relativistic X-ray jets in a galactic accreting source. The lobes are likely due to the interaction of relativistic plasma with the ISM. This ATCA proposal has allowed similar discovery in H 1743-322, and therefore that it maybe a common occurrence in the Galaxy. Recently, we have witnessed with ATCA the formation of similar lobes in the black hole GX 339-4. We propose to use the Compact Array to continue our search for radio lobes in microquasars that have been active in the past years.

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