The recurrent nova U Scorpii in the 1999 outburst: The first detection of a significant orbital-period change

Publications of the Astronomical Society of Japan

Volumn 55, Issue 1, 2003, Pages 297-304

  Matsumoto, Katsura ^a,c   Kato, Taichi ^a   Hachisu, Izumi ^b  

^a KYOTO UNIVERSITY   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c OKAYAMA UNIVERSITY   (Japan)

Author keywords

Accretion, accretion disks; Stars: individual: (U Scorpii); Stars: novae, cataclysmic variables

Indexed keywords

MASS TRANSFER; WHITE DWARFS;

ACCRETION: ACCRETION DISKS; BINARY SYSTEMS; LIGHT CURVES; OPTICAL-; ORBITAL PERIODS; SECONDARY ECLIPSE; STAR: INDIVIDUAL: (U SCORPII); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: NOVAE: CATACLYSMIC VARIABLES; TIME-RESOLVED; NOVAE CATACLYSMIC VARIABLES; STAR: INDIVIDUAL (U SCORPII);

SYSTEMS (METALLURGICAL);

EID: 0038743079     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/55.1.297     Document Type: Article

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