On the linewidth/K vs. mass ratio relation for SU Ursae Majoris stars and the removal of the inner disk

Astronomy and Astrophysics

Volumn 348, Issue 2, 1999, Pages 364-370

  Mennickent, R E ^a,b  

^a UNIVERSITY OF CONCEPCIÓN   (Chile)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Accretion, accretion disks; Methods: statistical stars: binaries: general; Stars: evolution; Stars: novae, cataclysmic variables

Indexed keywords

EID: 0008581617     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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