On the origin of the difference between the runaway velocities of the OB-supergiant x-ray binaries and the Be/x-ray binaries

Astronomy and Astrophysics

Volumn 364, Issue 2, 2000, Pages 563-572

  Van Den Heuvel, E P J ^a,c   Portegies Zwart, S F ^a,b   Bhattacharya, D ^d   Kaper, L ^a  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d RAMAN RESEARCH INSTITUTE   (India)

Author keywords

Stars: binaries: close; Stars: early type; Stars: emission line, Be; Stars: evolution; Stars: supernovae: general; X rays: stars

Indexed keywords

EID: 0000678716     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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