Modeling the Wind of the Be Star SS 2883
A. I. Bogomazov
TL;DR
This paper models the wind of the Be star SS 2883 using radio observations of pulsar eclipses, providing insights into stellar wind properties through numerical simulations.
Contribution
It introduces a numerical model of the Be-star wind based on eclipse observations, advancing understanding of stellar wind characteristics.
Findings
Consistent modeling of radio flux variations during eclipses
Quantitative estimates of free-free absorption in the stellar wind
Insights into the wind density and structure of SS 2883
Abstract
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.