A multi-wavelength study of the western lobe of W50 powered by the galactic microquasar SS 433

Advances in Space Research

Volumn 35, Issue 6, 2005, Pages 1062-1065

  Moldowan, A ^a   Safi Harb, S ^a   Fuchs, Y ^b   Dubner, G ^c  

^a UNIVERSITY OF MANITOBA   (Canada)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c INSTITUTO DE ASTRONOMÍA Y FÍSICA DEL ESPACIO   (Argentina)

Author keywords

Binaries: close; ISM: individual (W50); Radiation mechanisms: non thermal; Stars: individual (SS 433); Supernova remnants; X rays: stars

Indexed keywords

DATA REDUCTION; GALAXIES; IMAGE ANALYSIS; INFRARED RADIATION; MORPHOLOGY; SPECTROSCOPY; THERMAL EFFECTS; X RAYS;

BINARIES CLOSE; ISM: INDIVIDUAL (W50); NON-THERMAL; RADIATION MECHANISMS; STARS: INDIVIDUAL (SS 433); SUPERNOVA REMNANTS; X-RAYS: STARS;

COSMIC RAYS;

EID: 21744439353     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2005.01.086     Document Type: Conference Paper

References (10)

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