VLT spectroscopy and non-LTE modeling of the C/O-dominated accretion disks in two ultracompact X-ray binaries

Astronomy and Astrophysics

Volumn 450, Issue 2, 2006, Pages 725-733

  Werner, K ^a   Nagel, T ^a   Rauch, T ^a   Hammer, N J ^a,b   Dreizler, S ^c  

^a UNIVERSITY OF TÜBINGEN   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c UNIVERSITY OF GÖTTINGEN   (Germany)

Author keywords

Accretion, accretion disks; Binaries: close; Stars: individual: 4U 0614+091; Stars: individual: 4U 1626 67; X rays: binaries

Indexed keywords

ASTROPHYSICS; COMPUTER SIMULATION; HELIUM; MATHEMATICAL MODELS; OPTICAL RESOLVING POWER; RADIATION;

ACCRETION, ACCRETION DISKS; BINARIES: CLOSE; STARS: INDIVIDUAL: 4U 0614+091; X-RAYS: BINARIES;

X RAYS;

EID: 33646236329     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20053768     Document Type: Article

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