The nature of the close magnetic white dwarf + probable brown dwarf binary SDSS J121209.31+013627.7

Monthly Notices of the Royal Astronomical Society

Volumn 373, Issue 4, 2006, Pages 1416-1422

  Burleigh, M R ^a   Marsh, T R ^b   Gansicke B T ^b   Goad, M R ^a   Dhillon, V S ^c   Littlefair, S P ^c   Wells, M ^d   Bannister, N P ^a   Hurkett, C P ^a   Martindale, A ^a   Dobbie, P D ^a   Casewell, S L ^a   Baker, D E A ^a   Duke, J ^a   Farihi, J ^e   Irwin, M J ^f   Hewett, P C ^f   Roche, P ^g   Lewis, F ^g  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

^b UNIVERSITY OF WARWICK   (United Kingdom)

^c UNIVERSITY OF SHEFFIELD   (United Kingdom)

^d Oundle School   (United Kingdom)

^e GEMINI OBSERVATORY   (United States)

^f UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^g CARDIFF UNIVERSITY   (United Kingdom)

Author keywords

Novae, cataclysmic variables; Stars: low mass, brown dwarfs; White dwarfs

Indexed keywords

MAGNETISM;

ACCRETION RATE; BROWN DWARFS; DWARF BINARIES; MAGNETIC WHITE DWARFS; MOST LIKELY; NOVAE CATACLYSMIC VARIABLES; OPTICAL-; SHORT PERIODS; STARS: LOW-MASS BROWN DWARFS; TIMES SERIES;

WHITE DWARFS;

EID: 33845295128     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11030.x     Document Type: Article

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