Methods of asteroseismology for white dwarf stars

Details Methods of asteroseismology for white dwarf stars Methods of asteroseismology for white dwarf stars

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993balta...2..545b&link_type=abstract

Baltic Astronomy, vol. 2, p. 545

Astronomy and Astrophysics

Astronomy

8

Seismology, Astronomy, White Dwarf Stars, Stellar Oscillations, Stellar Interiors, Stellar Mass, Carbon, Nonlinearity

Scientific paper

A description of the various theoretical tools available for asteroseismology of white dwarf stars is given. These include period spacings between consecutive radial overtone g-modes, the mean of the period spacings, and mode trapping, as displayed by a period spacing diagram or the equivalent and frequency splittings within a multiplet for a given pulsation mode. Using PG 1159-035 and GD 358 as examples, I illustrate what we can learn from these stars when data of sufficient quality (from the Whole Earth Telescope, WET, for example) are available.

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