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An attempt of seismic modelling of β Cephei stars in NGC 6910

Published online by Cambridge University Press:  23 January 2015

D. Moździerski ,
Z. Kołaczkowski  and
E. Zahajkiewicz
D. Moździerski
Affiliation:
Asstronomical Institute, University of Wrocław, Kopernika 11, 51-622 Wrocław email: mozdzierski@astro.uni.wroc.pl
Z. Kołaczkowski
Affiliation:
Asstronomical Institute, University of Wrocław, Kopernika 11, 51-622 Wrocław email: mozdzierski@astro.uni.wroc.pl
E. Zahajkiewicz
Affiliation:
Asstronomical Institute, University of Wrocław, Kopernika 11, 51-622 Wrocław email: mozdzierski@astro.uni.wroc.pl
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Abstract

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We present preliminary results of seismic modeling of β Cephei-type stars in NGC 6910 based on simultaneous photometric and spectroscopic observations carried out in 2013 in Białków (photometry) and Apache Point (spectroscopy) observatories.

Keywords

stars: oscillationsopen clusters and associations: NGC 6910stars: early-typestars: fundamental parameters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 222 - 223
Copyright
Copyright © International Astronomical Union 2015 

References

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