Mode identification of multi-periodic Slowly Pulsating B-stars: results and problems

Details Mode identification of multi-periodic Slowly Pulsating B-stars: results and problems Mode identification of multi-periodic Slowly Pulsating B-stars: results and problems

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..189z&link_type=abstract

Communications in Astroseismology, Vol. 150, p.189

Astronomy and Astrophysics

Astronomy

5

Scientific paper

We report results from mode identifications (MI) for four selected multi-periodic Slowly Pulsating B-stars (SPB) using the Fourier parameter fit (FPF) method. Problems related to the pulsational nature of these objects which hamper a correct identification are discussed. For a present day status of knowledge about SPB stars we refer to De Cat (2007, this issue).

Affiliated with

Also associated with

No associations

Rating

Mode identification of multi-periodic Slowly Pulsating B-stars: results and problems 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 Mode identification of multi-periodic Slowly Pulsating B-stars: results and problems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mode identification of multi-periodic Slowly Pulsating B-stars: results and problems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-878249