XMM-Newton Proposal 02071102

Details XMM-Newton Proposal 02071102 XMM-Newton Proposal 02071102

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..362k&link_type=abstract

XMM-Newton Proposal ID #02071102

Computer Science

4U 1630-47, Xmm-Newton Proposal 02071102

Scientific paper

Microquasars are enigmatic binaries with a relativistic high-energy jet. Recently, the images of the jets of microquasars have been resolved with Chandra, that provides us a new way to investigate the jets; X-ray imaging. We propose an observation of three black-hole candidates, which 1) are considered to be microquasars based on their radio and X-ray activities, 2) experienced outbursts recently, probably accompanying a jet ejection, and 3) have not been observed with Chandra or XMM-Newton. Our purpose is to search for new microquasars by directly resolving their jet blobs and to determine the parameters of the proper motion and the shock.

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