The intricate optical line behaviour of the nova-like system V795 Herculis

Monthly Notices of the Royal Astronomical Society

Volumn 286, Issue 2, 1997, Pages 447-462

  Dickinson, R J ^a   Prinja, Raman K ^a   Rosen, S R ^b   King, A R ^b   Hellier, Coel ^c   Horne, Keith ^d  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c KEELE UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Binaries: close; Novae, cataclysmic variables

Indexed keywords

LIGHT EMISSION; NETWORK SECURITY; SEPARATION; WHITE DWARFS;

ACCRETION DISCS; BALMER LINES; BINARIES: CLOSE; EMISSION LINES; GAS STREAMS; HIGH VELOCITY; INNER CORE; NOVAE CATACLYSMIC VARIABLES; OPTICAL EMISSIONS; S-WAVES;

SPECTROGRAPHS;

EID: 0000380654     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/286.2.447     Document Type: Article

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