Determining temperature amplitude as a function of depth in the atmospheres of rapidly oscillating Ap stars

Monthly Notices of the Royal Astronomical Society

Volumn 299, Issue 2, 1998, Pages 371-378

  Medupe, R ^a,b   Kurtz, D W ^a  

^a UNIVERSITY OF CAPE TOWN   (South Africa)

^b AARHUS UNIVERSITY   (Denmark)

Author keywords

Stars: chemically peculiar; Stars: individual: HR 3831; Stars: individual: Cir; Stars: oscillations; Stars: variables: other

Indexed keywords

MODEL-BASED OPC; STAR OSCILLATIONS; STAR: INDIVIDUAL: HR 3831; STAR: INDIVIDUAL: Α CIR; STAR: VARIABLE: OTHER; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: VARIABLES; TEMPERATURE AMPLITUDE;

STARS;

EID: 0013202924     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01772.x     Document Type: Article

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