RAT J1953+1859: A dwarf nova discovered through high amplitude QPOs in quiescence

Monthly Notices of the Royal Astronomical Society

Volumn 398, Issue 3, 2009, Pages 1333-1338

  Ramsay, Gavin ^a   Hakala, Pasi ^b   Barclay, Thomas ^a,c   Wheatley, Peter ^d   Marshall, George ^d   Lehto, Harry ^b   Napiwotzki, Ralf ^e   Nelemans, Gijs ^f   Potter, Stephen ^g   Todd, Ian ^h  

^a ARMAGH OBSERVATORY   (United Kingdom)

^b UNIVERSITY OF TURKU   (Finland)

^c UNIVERSITY COLLEGE LONDON   (United Kingdom)

^d UNIVERSITY OF WARWICK   (United Kingdom)

^e UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^f RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^g SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^h QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

Author keywords

Accretion, accretion discs; Novae, cataclysmic variables; Stars: oscillations; Surveys; Techniques: photometric; X rays: binaries

Indexed keywords

PHOTOMETRY; RATS;

ACCRETION: ACCRETION DISKS; DWARF NOVAE; HIGH AMPLITUDES; ISAAC NEWTON TELESCOPE; NOVAE CATACLYSMIC VARIABLES; QUASIPERIODIC OSCILLATIONS; STAR OSCILLATIONS; TECHNIQUES: PHOTOMETRIC; TEMPORAL SURVEY; X-RAYS: BINARIES;

SURVEYS;

EID: 70249139491     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14982.x     Document Type: Article

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