What can we learn from the surface chemical composition of the optical companions of Soft X-ray transients?

Astronomy and Astrophysics

Volumn 374, Issue 1, 2001, Pages 195-203

  Ergma, E ^a,b   Sarna, M J ^c  

^a UNIVERSITY OF TARTU   (Estonia)

^b UNIVERSITY OF HELSINKI   (Finland)

^c NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

Author keywords

Stars: evolution; X ray: stars

Indexed keywords

EID: 0035401925     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010688     Document Type: Article

References (60)