Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-01-21
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
2 pages, 1 figure, to appear in Proceedings of IAU Symposium 259 "Cosmic Magnetic Fields: from Planets, to Stars and Galaxies"
Scientific paper
We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B stars. Roughly one third of the studied beta Cephei stars have detected magnetic fields. The fraction of magnetic Slowly Pulsating B and candidate Slowly Pulsating B stars is found to be higher, up to 50%. We find that the domains of magnetic and non-magnetic pulsating stars in the H-R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence.
Briquet Maryline
de Cat Peter
Hubrig Svetlana
Ilyin I. I.
Morel Th.
No associations
LandOfFree
New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars 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 New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-685044