Confirmation of the SU UMa-type nature of the suggested intermediate polar VZ pyxidis

Publications of the Astronomical Society of Japan

Volumn 49, Issue 4, 1997, Pages 481-484

  Kato, Taichi ^a   Nogami, Daisaku ^a  

^a KYOTO UNIVERSITY   (Japan)

Author keywords

Accretion disks; Stars: cataclysmic; Stars: dwarf novae; Stars: individual (VZ pyxidis)

Indexed keywords

STARS; MAGNETISM;

ACCRETION DISCS; DWARF NOVAE; INTERMEDIATE POLARS; NONMAGNETICS; PROPERTY; STAR: INDIVIDUAL (VZ PYXIDI); STARS: DWARF NOVAE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:CATACLYSMIC; TIME-RESOLVED;

MAGNETISM; STARS;

EID: 0031286753     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/49.4.481     Document Type: Article

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