X-Ray Binaries Part 2 - CYC3HIGH

Details X-Ray Binaries Part 2 - CYC3HIGH X-Ray Binaries Part 2 - CYC3HIGH

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.5082b&link_type=abstract

HST Proposal ID #5082

Astronomy and Astrophysics

Astrophysics

Hst Proposal Id #5082

Scientific paper

The extreme conditions existing in the near vicinity of neutron stars which are the secondaries in close binaries provide a laboratory in which we may observationally confirm or refine many of our basic theories of astrophysics. This program will monitor the photometric and polarimetric light curves of X-ray binaries at several different phases of the binary orbit in several different wavelength bands in the UV. The results will be related to the structure of, and physical conditions existing in, the gas streams (and possibly, the accretion disk) in these systems. Revision History: Clone 2958 v1.1 Removed comments concerning POL tube calibration-- BJW 6/24/92; Removed HDE226868 (MJT 6/2/93).

Affiliated with

Also associated with

No associations

Rating

X-Ray Binaries Part 2 - CYC3HIGH 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 X-Ray Binaries Part 2 - CYC3HIGH, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-Ray Binaries Part 2 - CYC3HIGH will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1071855