Mass Exchange Binaries (fos 34) SS 2883 : Cycle 3

Details Mass Exchange Binaries (fos 34) SS 2883 : Cycle 3 Mass Exchange Binaries (fos 34) SS 2883 : Cycle 3

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.5199m&link_type=abstract

HST Proposal ID #5199

Astronomy and Astrophysics

Astronomy

Hst Proposal Id #5199

Scientific paper

FOS UV spectroscopy will be used to study the Be star (SS 2883; CD-63D2495) binary companion to the pulsar PSR1259-63. The pulsar is eclipsed near periastron, due to the wind of the Be star, and or a circumstellar disk. UV spectra near periastron will be used to probe the Be star wind and disk material, and perhaps their interaction with the pulsar.

Affiliated with

Also associated with

No associations

Rating

Mass Exchange Binaries (fos 34) SS 2883 : Cycle 3 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 Mass Exchange Binaries (fos 34) SS 2883 : Cycle 3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass Exchange Binaries (fos 34) SS 2883 : Cycle 3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1071867