Multimode Radiative beta Cephei and delta Cephei Models

Details Multimode Radiative beta Cephei and delta Cephei Models Multimode Radiative beta Cephei and delta Cephei Models

2008-03-10

arxiv.org/abs/0803.1441v1

EAS Publ. Ser. 38: 175-183, 2009

Astronomy and Astrophysics

Astrophysics

to appear in the proceedings of the "Nonlinear stellar hydrodynamics", conference in honor of Robert Buchler's 65 birthday, 9-

Scientific paper

10.1051/eas/0938019

As a by-product of beta Cephei and delta Cephei radiative model surveys we have found interesting cases of multimode pulsation. In case of beta Cephei stars, we found two multimode domains with two or three modes being involved. The origin of the multimode pulsation can be traced to one of the two different mechanisms: either to the non-resonant coupling of the two excited modes (double-mode pulsation) or to the 2omega_1 = omega_0 + omega_2 parametric resonance (triple-mode pulsation). In case of delta Cephei models, a triple-mode pulsation domain, connected with the 2:1 resonance, 2omega_0 = omega_2, is found. These models are of theoretical interest only, since they do not obey a proper mass-luminosity relation.

Affiliated with

Also associated with

No associations

Rating

Multimode Radiative beta Cephei and delta Cephei Models 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 Multimode Radiative beta Cephei and delta Cephei Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multimode Radiative beta Cephei and delta Cephei Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-379175