High Resolution X-Ray Spectroscopy of the Precessing Jet in SS 433 (part Iii)

Details High Resolution X-Ray Spectroscopy of the Precessing Jet in SS 433 (part Iii) High Resolution X-Ray Spectroscopy of the Precessing Jet in SS 433 (part Iii)

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..459c&link_type=abstract

Chandra Proposal ID #02400069

Physics

Chandra Proposal Id #02400069

Scientific paper

SS 433 is quite a unique galactic X-ray binary. The X-ray emission from emerging jets are of thermal origin. The cooling hydrodynamical outflow in form of a jet has dimensions of the binary separation. SS 433 has been observed during AO1 for 30 ks revealing a variety of redshifted and blue shifted lines from Si and higher elements. The line ratios of various H/He-like ions as well as deduced temperatures differed considerably from what has been observed with ASCA during approximately the same phase. We intend to observe SS 433 at several more precession phases (part III: eclipse) in order to monitor the plasmas conditions at the base of the jet as well as measure the X-ray Doppler shifts of the lines from the precessing jet.

Affiliated with

Also associated with

No associations

Rating

High Resolution X-Ray Spectroscopy of the Precessing Jet in SS 433 (part Iii) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High Resolution X-Ray Spectroscopy of the Precessing Jet in SS 433 (part Iii), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Resolution X-Ray Spectroscopy of the Precessing Jet in SS 433 (part Iii) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1524969