2001/12/14 by Yael Fuchs, Yaël Fuchs, Fuchs, Yael
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Gamma-ray bursts and supernovae #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0112344
4 pages, 3 figures, Proceedings of "Semaine de l'Astrophysique Francaise", meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: Societe Francaise d'Astronomie et d'Astrophysique, to be published by EdP-Sciences, Conference Series
arxiv created 2001/12/14 · openalex publication_date 2001/12/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
SS433 is a jet emitting X-ray binary surrounded by the W50 radio nebula. The SS433/W50 system is an excellent laboratory for studying relativistic jet interaction with the surrounding interstellar medium. In this context, part of the W50 nebula has been mapped with ISOCAM at 15 micron. I will show the results particularly on the W50 west lobe, and on 2 emitting zones detected with IRAS who have also been observed in millimetre wavelength (CO(1-0) transition), and for one of them by spectroscopy with ISOLWS and ISOSWS between 2 and 200 micron.