Amplitude variability or close frequencies in pulsating stars - The δ Scuti star FG Vir

Monthly Notices of the Royal Astronomical Society

Volumn 368, Issue 2, 2006, Pages 571-578

  Breger, M ^a   Pamyatnykh, A A ^a,b,c  

^a Institut fur Astronomie Vienna   (Austria)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^c INSTITUTE OF ASTRONOMY   (Russian Federation)

Author keywords

Stars: individual: FG Vir; Stars: oscillations; Techniques: photometric; Scuti

Indexed keywords

PHOTOMETRY; STARS;

AMPLITUDE VARIABILITY; AMPLITUDE VARIATIONS; INDIVIDUAL:FG VIR; PHASE VARIATION; SCUTI STARS; STAR OSCILLATIONS; STAR: INDIVIDUAL: FG VIR; STARS: INDIVIDUAL: PROXIMA CENTAURI; TECHNIQUES: PHOTOMETRIC; Δ SCUTI;

POWER SPECTRUM;

EID: 33646242751     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10119.x     Document Type: Article

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