The orbital period of the SU Ursae Majoris star EK Trianguli Australis and evidence for ring-like accretion disks in long-supercycle length SU Ursae Majoris stars

Publications of the Astronomical Society of Japan

Volumn 50, Issue 3, 1998, Pages 333-342

  Mennickent, Ronald E ^a   Arenas, Jose ^a  

^a UNIVERSITY OF CONCEPCIÓN   (Chile)

Author keywords

Accretion; Evolution; Stars: Cataclysmic; Stars: Dwarf novae; Stars: Individual (WX Ceti, AK Cncri, AQ Eridani, RZ Leonis, TU Mensae, EK Trianguli Australis, CU Velorum, WZ Sagittae); Stars: Variable

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; MAGNETOSPHERE; MASS TRANSFER;

ACCRETION; ACCRETION DISCS; EMISSION LINES; EVOLUTION; ORBITAL PERIODS; STAR: INDIVIDUAL (WX CETI, AK CNCRI, AQ ERIDANI, RZ LEONIS, TU MENSAE, EK TRIANGULUS AUSTRALI, CU VELORUM, WZ SAGITTAE); STARS: DWARF NOVAE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: VARIABLES; STARS:CATACLYSMIC; STAR: INDIVIDUAL (WX CETI, AK CNCRI, AQ ERIDANI, RZ LEONIS, TU MENSAE, EK TRIANGUU AUSTRALI, CU VELORUM, WZ SAGITTAE);

WHITE DWARFS;

EID: 0032325773     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/50.3.333     Document Type: Article

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