The photometric method of mode identification for rapidly rotating SPB stars. An application to μ Eridani

Details The photometric method of mode identification for rapidly rotating SPB stars. An application to μ Eridani The photometric method of mode identification for rapidly rotating SPB stars. An application to μ Eridani

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.118a2024d&link_type=abstract

Journal of Physics: Conference Series, Volume 118, Issue 1, pp. 012024 (2008).

Physics

Scientific paper

We present an outline of a method for mode identification, which relies on a nonadiabatic version of the traditional approximation and involves instability and visibility considerations. Determination of the angular degrees, (l, m), is done simultaneously with the rotation velocity and inclination angle. The method is applied to oscillation frequencies detected in the rapidly rotating SPB star μ Eridani.

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