Linear nonradial pulsation theory. Lecture 7
Conference
·
OSTI ID:6168611
Many of the upper main-sequence stars pulsate in spheroidal nonradial modes. We know this to be true in numerous cases, as we have tabulated for the ..beta.. Cephei and delta Scuti variables in previous lectures. However, we cannot identify the actual mode for any star except for the low-order pressure p and f modes of our sun. It remains a great challenge to clearly state what really is occurring, in the process we learn more about how stars evolve and pulsate.
- Research Organization:
- Los Alamos National Lab., NM (USA)
- DOE Contract Number:
- W-7405-ENG-36
- OSTI ID:
- 6168611
- Report Number(s):
- LA-UR-83-787; CONF-830337-6; ON: DE83010090
- Country of Publication:
- United States
- Language:
- English
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