Orbital periods of cataclysmic variables identified by the SDSS - V. VLT, NTT and Magellan observations of nine equatorial systems

Monthly Notices of the Royal Astronomical Society

Volumn 391, Issue 2, 2008, Pages 591-606

  Southworth, John ^a   Gansicke B T ^a   Marsh, T R ^a   Torres, M A P ^b   Steeghs, D ^a,b   Hakala, P ^c   Copperwheat, C M ^a   Aungwerojwit, A ^a,d   Mukadam, A ^e  

^a UNIVERSITY OF WARWICK   (United Kingdom)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF TURKU   (Finland)

^d NARESUAN UNIVERSITY   (Thailand)

^e UNIVERSITY OF WASHINGTON   (United States)

Author keywords

Binaries: spectroscopic; Novae, cataclysmic variables; Stars: dwarf novae; White dwarfs

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GALAXIES; LUMINANCE; MASS TRANSFER; TELESCOPES;

BINARIES: SPECTROSCOPIC; CATACLYSMIC VARIABLES; EMISSION LINES; HΑ EMISSION; MAGELLAN; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; SLOAN DIGITAL SKY SURVEY; STARS: DWARF NOVAE; VERY LARGE TELESCOPE;

WHITE DWARFS;

EID: 57149134282     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13932.x     Document Type: Article

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