University of Cambridge > Talks.cam > Institute of Astronomy Colloquia > Tuning stellar cores from gravity modes detected in CoRoT and Kepler data of various types of stars

Tuning stellar cores from gravity modes detected in CoRoT and Kepler data of various types of stars

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Dr. Vasily Belokurov.

The CoRoT and Kepler space missions, while still ongoing, already revolutionised our view on stellar pulsation. In this talk, we illustrate how the immense advantage of having long-term uninterrupted data from space with a factor 100 better precision compared to data from the ground implies large progress in the tuning of stellar physics. In particular, we focus on the cases where gravity-mode oscillations were detected and allowed modelling of the near-core regions in stars. We end by highlighting future prospects based on the continuing data gathering by both missions.

This talk is part of the Institute of Astronomy Colloquia series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

© 2006-2020 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity