Spectroscopic evidence for the binary nature of AM CVn

Monthly Notices of the Royal Astronomical Society

Volumn 326, Issue 2, 2001, Pages 621-627

  Nelemans, G ^a   Steeghs, D ^b   Groot, P J ^c  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Accretion, accretion discs; Binaries: close; Binaries: spectroscopic; Novae, cataclysmic variables; Stars: individual: AM CVn

Indexed keywords

STARS;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BINARIES: SPECTROSCOPIC; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; S-WAVES; SPECTROSCOPIC DATA; SPECTROSCOPIC EVIDENCE; STAR: INDIVIDUAL: AM CVN; STARS: INDIVIDUAL: PROXIMA CENTAURI;

SHEAR WAVES;

EID: 0011298409     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04614.x     Document Type: Article

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