`Star as a sun' observations in seismology of distant stars

Details `Star as a sun' observations in seismology of distant stars `Star as a sun' observations in seismology of distant stars

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..152..275m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 152, no. 1, p. 275-282

Physics

9

Doppler Effect, Helioseismology, Line Spectra, Pulsed Radiation, Stellar Oscillations, Stellar Rotation, Stellar Spectrophotometry, Abundance, Chemical Analysis, Stellar Composition, Stellar Models

Scientific paper

This paper gives a brief description of a new procedure for seismology of pulsating CP2-stars. In analogy with the solar observations, this sensitive procedure permits one to carry out the spatial filtration of low, intermediate and high degree nonradial modes and uses periodic spatial filters associated with surface inhomogenities in the distribution of chemical elements. The possibilities of this procedure and its observational peculiarities are discussed.

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