Application of two-time methods in stellar pulsations

Details Application of two-time methods in stellar pulsations Application of two-time methods in stellar pulsations

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8324441p&link_type=abstract

Presented at the Conf. on Pulsations in Classical and Cataclysmic Variables, Boulder, Colo., 1-4 Jun. 1982

Physics

Cepheid Variables, Pulses, Stellar Evolution, Stellar Models, Asymptotic Methods, Eigenvectors, Nonadiabatic Conditions

Scientific paper

The method of two time expansions is extended to include the effects of the outer, nonadiabatic layers in stellar pulsation. The evolution of pulsating stellar models can be examined, including the approach to limit cycle behavior. The method is demonstrated by a calculation of the eigenvectors for a beta Cepheid model. It is argued that the method is promising as a practical tool for treating the approach to limiting oscillations, as well as resonant and multimode behavior.

Affiliated with

Also associated with

No associations

Rating

Application of two-time methods in stellar pulsations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Application of two-time methods in stellar pulsations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Application of two-time methods in stellar pulsations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1024760