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Spectroscopical analysis of δ Scuti stars

Published online by Cambridge University Press:  26 May 2016

E. Solano  and
J. Fernley
E. Solano
Affiliation:
VILSPA-INSA. P.O. Box 50727. 28080 Madrid (Spain)
J. Fernley
Affiliation:
VILSPA-ESA. P.O. Box 50727. 28080 Madrid (Spain)

Extract

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δ Scuti are pulsating stars with a characteristic period of several hours, lying in the A2-F5 spectral range and placed on or a little above the main sequence. Unlike the well-known “classical” RR Lyrae or Cepheids, which show a homogeneous pulsational behaviour (i.e. radial modes with large amplitudes), δ Scuti stars have peculiarities: their amplitudes vary from millimagnitudes to tenths of magnitude and their pulsation modes can be both radial and non-radial.

Type
1. Pulsation and Rotation
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 47 - 48
Copyright
Copyright © Kluwer 1994 

References

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