Spectroscopic modelling of non-radial pulsation in rotating early-type stars
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645 citations
Cites methods from "Spectroscopic modelling of non-radi..."
...Townsend (1997) published a modeling code applicable to NRP in rapidly rotating stars in general, i.e., not only to Be stars, the BRUCE/KYLIE package....
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Cites methods from "Spectroscopic modelling of non-radi..."
...The calculations use the bruce code (Townsend 1997), which is readily adapted from its original intended application in modeling nonradial pulsation by simply setting the pulsation amplitudes to zero....
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Cites background or methods from "Spectroscopic modelling of non-radi..."
...The ( , m) pair of indices is often used to classify the Hough functions (e.g. Townsend 1997a,b), as it provides a clear indication of their nonrotating progenitors....
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...Such an ordering is always possible, because the eigenvalues of the tidal equation are guaranteed never to be degenerate (see, e.g. Townsend 1997a,b)....
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...…applied in many areas of stellar pulsation, from modelling the nrp-originated line-profile variations seen in early-type stars (Lee & Saio 1990; Townsend 1997b), to examining tidal forcing in massive binary systems (Papaloizou & Savonije 1997), to investigating what role gravity modes might…...
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