Observable quantities of nonradial pulsations in the presence of slow rotation

Details Observable quantities of nonradial pulsations in the presence of slow rotation Observable quantities of nonradial pulsations in the presence of slow rotation

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...292..238p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 292, May 1, 1985, p. 238-248.

Astronomy and Astrophysics

Astrophysics

51

Early Stars, Power Spectra, Stellar Motions, Stellar Oscillations, Stellar Rotation, White Dwarf Stars, Limb Darkening, Main Sequence Stars, Radial Velocity

Scientific paper

Theoretical power spectra of both light and radial velocity variations of a nonradially pulsating star that include the effects of rotation are presented. Three classes of motion are defined, depending on the symmetry of the mode of interest and its orientation with respect to the rotating axis. The use of tabulated model atmospheres to predict color variations is compared to the blackbody approximation for two cases, a hydrogen white dwarf (DA) and a main-sequence B Star.

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