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Solar-like stars seismology

Published online by Cambridge University Press:  26 February 2010

Dumitru Pricopi
Affiliation:
Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint 5, RO-040557 Bucharest, Romania emails: [email protected], [email protected]
Marian Doru Suran
Affiliation:
Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint 5, RO-040557 Bucharest, Romania emails: [email protected], [email protected]
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Abstract

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Many solar like stars were observed by CoRoT and MOST missions. We try to investigate some of these stars using asteroseismic inversion method using both frequencies fitting and separation fitting. Our results are compared with semiempirical method based on direct power spectrum analysis.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

del Peloso, E. F., Cunha, K., da Silva, L., & Porto de Mello, G. F. 2005, A&A, 441, 1149Google Scholar
Grevesse, N. & Noels, A. 1993, Cosmic abundance of the elements, in Origin and evolution of the elements, edited by Prantzos, N., Vangioni Flam, E. and Casse, M., Cambridge University, England, pp. 1525Google Scholar
Jonsell, K., Edvardsson, B., Gustafsson, B. et al. 2005, A&A, 440, 231Google Scholar
Mosser, B., Deheuvels, S., Michel, E. et al. 2008, A&A (to appear)Google Scholar
Thevenin, F. 1998 VisieR Online Data Catalog, 3193, 0Google Scholar