Radial and Nonradial Oscillations of 63 Her (HD155514 = HR6391)

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Stars: 63 Her, Pulsations, Evolution

Scientific paper

An attempt has been made toward explaining the observed frequencies in 63 Her. A sequence of evolutionary models have been calculated up to a point where stellar parameters match the observed luminosity and effective temperature of 63 Her. Radial and nonradial oscillations frequencies were obtained for a series of masses 1.85, 1.90 and 1.95 M&sun; and eigth models which represent best the pulsations of 63 Her are given in this paper. Calculations are restricted to low harmonic degrees ( l= 0,1,2,3 ). Six of the eigth observed frequencies quoted in literature were obtained. These we obtained for the model of mass 1.90 M&sun;. The observationally measured frequency 220.7 m Hz, which is classified as a second harmonic radial oscillation, and five of the observed nonradial modes were obtained at the harmonic degree l=3. The difference between the observed and calculated frequencies are (nn/l,c - nobs)= 0.3, 0.8, 0.7, 0.2, and 0.7 m Hz with n/l= -15/3, -12/3, -9/3, -7/3, -3/3, respectively.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Radial and Nonradial Oscillations of 63 Her (HD155514 = HR6391) 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 Radial and Nonradial Oscillations of 63 Her (HD155514 = HR6391), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial and Nonradial Oscillations of 63 Her (HD155514 = HR6391) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-834132

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.