The detection of the rich p-mode spectrum and asteroseismology of Przybylski's star

Astronomy and Astrophysics

Volumn 490, Issue 3, 2008, Pages 1109-1120

  Mkrtichian, D E ^a,b   Hatzes, A P ^c   Saio, H ^d   Shobbrook, R R ^e  

^a Sejong University   (South Korea)

^b ODESSA NATIONAL UNIVERSITY   (Ukraine)

^c THÜRINGER LANDESSTERNWARTE TAUTENBURG   (Germany)

^d TOHOKU UNIVERSITY   (Japan)

^e AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

Stars: chemically peculiar; Stars: individual: HD 101065; Stars: oscillations

Indexed keywords

CHEMICAL ANALYSIS; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC MATERIALS; OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; PHOTOGRAPHY; PHOTOMETRY; STARS; TELESCOPES;

ASTEROSEISMOLOGY; AXISYMMETRIC; BEST FITTEST; CHEMICAL COMPOSITIONS; DIPOLE MAGNETIC FIELDS; EFFECTIVE TEMPERATURES; IN PHASES; LARGE SPACINGS; LIGHT CURVES; MAGNETIC; MODE SPECTRUMS; NONADIABATIC; OSCILLATION FREQUENCIES; OSCILLATION MODES; OSCILLATION SPECTRUMS; P-MODES; PHOTOMETRIC DATUM; RADIAL VELOCITIES; RANGING; SEQUENCE MODELS; SPECTRAL LINES; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: HD 101065; STARS: OSCILLATIONS; STELLAR PARAMETERS; SURFACE GRAVITIES; WAVELENGTH RANGES;

THERMAL LOGGING;

EID: 54949123100     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809890     Document Type: Article

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