The Evolution of the fossil Jets associated with 4U1755-33

Details The Evolution of the fossil Jets associated with 4U1755-33 The Evolution of the fossil Jets associated with 4U1755-33

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cxo..prop.1438a&link_type=abstract

Chandra Proposal ID #05401015

Physics

Chandra Proposal Id #05401015

Scientific paper

4U1755-33 had been a bright persistent source for at least 25 yrs, but in 1995 entered an extended quiescent phase. An XMM-Newton observation of 4U1755-33, made to study the quiscence emission, reveals the presence of a narrow 7' long X-ray jet-like feature centered on the position of 4U1755-33. This is the second LMXRB that shows evidence of an X-ray ray jet. We propose to use the high angular resolution of Chandra to study the jet morphology and evolution with time. This observation will also place a factor of 10 improved upper limit on the quiscence emission of 4U1755-33, and place further constraints on whether or not this system contains a black hole.

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