An alternative to O - C analysis of variable star periods

Monthly Notices of the Royal Astronomical Society

Volumn 294, Issue 4, 1998, Pages 657-666

  Lombard, F ^a  

^a UNIVERSITY OF JOHANNESBURG   (South Africa)

Author keywords

Methods: data analysis; Methods: statistical; Stars: individual: RY Sgr; Stars: individual: X Aur; Stars: variables: other

Indexed keywords

AUTOCORRELATION; FREQUENCY DOMAIN ANALYSIS;

AUTO CORRELATION; METHODS. DATA ANALYSIS; METHODS:STATISTICAL; STAR: INDIVIDUAL: RY SGR; STAR: INDIVIDUAL: X AUR; STAR: VARIABLE: OTHER; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: VARIABLES; VARIABLE STARS;

STARS;

EID: 0005878759     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-8711.1998.01214.x     Document Type: Article

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