On the frequency and amplitude variations of the δ Scuti star CD-24 7599 (=XX Pyx)

Monthly Notices of the Royal Astronomical Society

Volumn 295, Issue 2, 1998, Pages 377-385

  Handler, G ^a,h,i   Pamyatnykh, A A ^a,b,c   Zima, W ^a,j   Sullivan, D J ^d   Audard, N ^e,f,h   Nitta, A ^g  

^a UNIVERSITY OF VIENNA   (Austria)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^c INSTITUTE OF ASTRONOMY   (Russian Federation)

^d VICTORIA UNIVERSITY OF WELLINGTON   (New Zealand)

^e UNIVERSITÉ CÔTE D'AZUR   (France)

^f UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^g UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^h University of Texas at Austin   (United States)

ⁱ SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^j CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

more..

Author keywords

Stars: Individual: CD 24 7599; Stars: Individual: XX Pyx; Stars: Oscillations; Techniques: Photometric; Scuti

Indexed keywords

MAGNETIC FIELD EFFECTS; PHOTOMETRY; STARS;

AMPLITUDE VARIATIONS; FREQUENCY VARIATION; SCUTI STARS; STAR OSCILLATIONS; STAR: INDIVIDUAL: CD-24 7599; STAR: INDIVIDUAL: XX PYX; STARS: INDIVIDUAL: PROXIMA CENTAURI; TECHNIQUES: PHOTOMETRIC; Δ SCUTI;

AMPLITUDE MODULATION;

EID: 0002658872     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01208.x     Document Type: Article

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