The superluminal source GRS 1915+105: A high-mass X-ray binary?

Astrophysical Journal

Volumn 477, Issue 1 PART II, 1997, Pages

  Mirabel, I F ^a,b   Bandyopadhyay, R ^c   Charles, P A ^c   Shahbaz, T ^c   Rodriguez L F ^d  

^a CEA SACLAY   (France)

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

^c UNIVERSITY OF OXFORD   (United Kingdom)

^d UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Infrared: stars; Stars: emission line, Be; X rays: stars

Indexed keywords

EID: 21744444115     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310509     Document Type: Article

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