On the Possibility of V4444 Sgr as a Recurrent Nova

Publications of the Astronomical Society of Japan

Volumn 56, Issue SPEC. ISS. 1, 2004, Pages

  Kato, Taichi ^a   Yamaoka, Hitoshi ^b   Kiyota, Seiichiro ^c  

^a KYOTO UNIVERSITY   (Japan)

^b KYUSHU UNIVERSITY   (Japan)

^c Variable Star Observers League Japan   (Japan)

Author keywords

Astrometry; Stars: individual (V4444 Sagittarii); Stars: novae, cataclysmic variables; Stars: variable

Indexed keywords

ASTROMETRY; CLASSICAL NOVAE; LIGHT CURVES; PHOTOMETRICS; SPECTRA'S; STAR: INDIVIDUAL (V4444 SAGITTARII); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: NOVAE: CATACLYSMIC VARIABLES; STARS: VARIABLES; CATACLYSMIC VARIABLES; STARS:NOVAE;

STARS;

EID: 1942537059     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/56.sp1.s83     Document Type: Article

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