X-Ray Jets in Microquasars

Details X-Ray Jets in Microquasars X-Ray Jets in Microquasars

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1669c&link_type=abstract

Chandra Proposal ID #06400159

Physics

Chandra Proposal Id #06400159

Scientific paper

We propose Target of Opportunity (ToO) observations for detailed studies of X-ray jets from microquasars. We describe our discovery of radio/X-ray jets in two microquasars and why X-ray jets are probably much more common than previously thought and also why it offers an exciting new way to probe the physics of the jets. The proposed ToO observations are optimized to discover and study (flux evolution, morphology, SED, proper motion, ...) new X-ray jets from microquasars, based on their detection as radio lobes. This will have implications not only for the study of jets from Galactic X-ray binaries, but also for our understanding of relativistic jets from active galactic nuclei (AGN).

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