Modeling the Wind of the Be Star SS 2883

Details Modeling the Wind of the Be Star SS 2883 Modeling the Wind of the Be Star SS 2883

2008-06-30

arxiv.org/abs/0806.4868v1

Astron.Rep.49:709-713,2005

Astronomy and Astrophysics

Astrophysics

6 pages, 7 figures

Scientific paper

10.1134/1.2045321

Observations of eclipses of the radio pulsar B1259-63 by the disk of its Be-star companion SS 2883 provide an excellent opportunity to study the winds of stars of this type. The eclipses lead to variations in the radio flux (due to variations in the free-free absorption), dispersion measure, rotation measure, and linear polarization of the pulsar. We have carried out numerical modeling of the parameters of the Be-star wind and compared the results with observations.

Affiliated with

Also associated with

No associations

Rating

Modeling the Wind of the Be Star SS 2883 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 Modeling the Wind of the Be Star SS 2883, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the Wind of the Be Star SS 2883 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-154904