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27 April 2024
 
  » arxiv » astro-ph/0112339

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A 2.4-80 micron spectrophotometric study of SS433 with ISO
Yael Fuchs ; Lydie Koch-Miramond ; Peter Abraham ;
Date 14 Dec 2001
Subject astro-ph
Affiliation2 and 3) ( Service d’Astrophysique CEA/Saclay France, Konkoly Observatory Budapest Hungary, MPIA Heidelberg Germany
AbstractWe 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.
Source arXiv, astro-ph/0112339
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