Pulsation in the atmosphere of roAp stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

invited review presented at HELAS Wroclaw Workshop Interpretation of Asteroseismic Data, Communications in Asteroseismology, i

Scientific paper

High time resolution spectroscopy of roAp stars at large telescopes has led to a major breakthrough in our understanding of magnetoacoustic pulsations in these interesting objects. New observations have allowed to uncover a number of intricate relations between stellar oscillations, magnetic field, and chemical inhomogeneities. It is now understood that unusual pulsational characteristics of roAp stars arise from an interplay between short vertical length of pulsation waves and extreme chemical stratification. Here I review results of recent studies which utilize these unique properties to map 3D pulsation geometry using a combination of Doppler imaging, vertical pulsation tomography, interpretation of line profile variation, and ultraprecise space photometry. I also describe recent attempts to interpret theoretically the complex observational picture of roAp pulsations.

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

Pulsation in the atmosphere of roAp 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 Pulsation in the atmosphere of roAp stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsation in the atmosphere of roAp stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-30672

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