A 2.4-80 micron spectrophotometric study of SS433 with ISO
Astrophysics
2007-05-23 v1
Abstract
We present ISOPHOT spectrophotometric observations of SS433 at four different orbital phases in 1996 and 1997. The HeI+HeII lines in both spectra of SS433 and the Wolf-Rayet star WR147, a WN8+BO5 binary system, closely match. The 2.5-12 micron continuum radiation is due to an expanding wind free-free emission in an intermediate case between optically thick and optically thin regime. A rough mass loss rate evaluation gives about 1.4 10^{-4} M_sun/yr. Results are consistent with a Wolf-Rayet-like companion to the compact object in SS433.
Cite
@article{arxiv.astro-ph/0112339,
title = {A 2.4-80 micron spectrophotometric study of SS433 with ISO},
author = {Yael Fuchs and Lydie Koch-Miramond and Peter Abraham},
journal= {arXiv preprint arXiv:astro-ph/0112339},
year = {2007}
}
Comments
4 pages, 2 figures, to appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M. Gaensler