Modelling pulsation amplitudes of ξ Hydrae

Details Modelling pulsation amplitudes of ξ Hydrae Modelling pulsation amplitudes of ξ Hydrae

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.336l..65h&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 336, Issue 4, pp. L65-L69.

Astronomy and Astrophysics

Astronomy

51

Convection, Stars: Individual: Ξ Hya, Stars: Oscillations

Scientific paper

Amplitudes of stochastically excited oscillations of models of ξ Hydrae (HR4450) are presented. The theoretical results are compared with the recent measurements by an international group of astronomers announced in the ESO press release 10/02. Using a stochastic excitation model we find fair agreement between estimated velocity amplitudes and the values quoted in the ESO press release.

Affiliated with

Also associated with

No associations

Rating

Modelling pulsation amplitudes of ξ Hydrae 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 Modelling pulsation amplitudes of ξ Hydrae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modelling pulsation amplitudes of ξ Hydrae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-950596