Mapping the Jets of SS 433

Details Mapping the Jets of SS 433 Mapping the Jets of SS 433

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..591n&link_type=abstract

Chandra Proposal ID #02400911

Physics

Chandra Proposal Id #02400911

Scientific paper

ASCA revealed Doppler-shifted emission lines in its X-ray spectrum originating from the two anti-parallel jets. The ASCA data indicated the X-ray jet is ˜10(13) cm long te{Kotani97a}, ten times longer than the previous estimations (e.g., te{Stewart87}, te{Watson86}). The data also suggest the existence of an absorber, a disk outflow and/or matter distributed in the orbital plain te{Kotani96}. Our proposal is to reveal the violent outflow/inflow of SS 433, which is the only system ever know to be in a steady super-critical accretion state, and to explore the nature of it.

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