Nonradial pulsations in early-type B stars - g-modes or r-modes

Details Nonradial pulsations in early-type B stars - g-modes or r-modes Nonradial pulsations in early-type B stars - g-modes or r-modes

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254..708s&link_type=abstract

Astrophysical Journal, Part 1, vol. 254, Mar. 15, 1982, p. 708-712.

Astronomy and Astrophysics

Astrophysics

7

B Stars, Early Stars, Light Curve, Planetary Waves, Stellar Oscillations, Variable Stars, Coriolis Effect, Radial Velocity, Spherical Waves, Velocity Distribution

Scientific paper

A variety of considerations suggest that the nonradial oscillations
present in 53 Per stars and several β Cep stars do not arise from
Rossby (r-) waves, but rather from spheroidal waves, such as g-modes.

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