The γ Dor variable HR 8799: Results from a multisite campaign

Monthly Notices of the Royal Astronomical Society

Volumn 303, Issue 2, 1999, Pages 275-283

  Zerbi, F M ^a   Rodriguez E ^b   Garrido, R ^b   Martin S ^b   Arellano Ferro, A ^c   Sareyan, J P ^d   Krisciunas, K ^e   Akan, M C ^f   Evren, S ^f   Ibanoglu C ^f   Keskin, V ^f   Pekunlu R ^f   Tunca, Z ^f   Luedeke, K ^g   Paparo M ^h   Nuspl, J ^h   Guerrero, G ^a  

^a INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^b INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^c UNIVERSITY OF GUANAJUATO   (Mexico)

^d UNIVERSITÉ CÔTE D'AZUR   (France)

^e UNIVERSITY OF WASHINGTON   (United States)

^f EGE UNIVERSITY   (Turkey)

^g Konkoly Observatory ^*  (United States)

^h KONKOLY OBSERVATORY   (Hungary)

Author keywords

Stars: individual: HR 8799; Stars: oscillations; Stars: variables: other

Indexed keywords

AMPLITUDE MODULATION; STARS; STOCHASTIC MODELS; STOCHASTIC SYSTEMS;

COUPLING TERMS; MULTI-SITE; PHOTOMETRICS; SIGNIFICANCE LEVELS; STAR OSCILLATIONS; STAR: INDIVIDUAL: HR 8799; STAR: VARIABLE: OTHER; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: VARIABLES; TYPE VARIABLES;

PHOTOMETRY;

EID: 0001202861     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02209.x     Document Type: Article

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