Results of the ensemble asteroseismology of B-type stars in open cluster NGC 6910
Abstract
We present the results of ensemble asteroseismology of B-type pulsating stars in the NGC 6910 open cluster. Ensemble asteroseismology turns out to be very useful for examination of the instability strip, mode identification and testing the excitation of the modes. It also helps to constrain parameters of the cluster, its age in particular. The outcome shows the large potential of this method, especially when used with space telescopes, e.g. Kepler or TESS, that can provide precise photometry for cluster members.
- Publication:
-
Stars and their Variability Observed from Space
- Pub Date:
- 2020
- Bibcode:
- 2020svos.conf..341M
- Keywords:
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- asteroseismology;
- stars: fundamental parameters;
- open clusters and associations: individual: NGC 6910