Asteroseismic analysis of the CoRoT target HD 169392
| Autor: | Mathur, S., Bruntt, H., Catala, C., Benomar, O., Davies, G. R., Garcia, R. A., Salabert, D., Ballot, J., Mosser, B., Regulo, C., Chaplin, W. J., Elsworth, Y., Handberg, R., Hekker, S., Mantegazza, L., Michel, E., Poretti, E., Rainer, M., Roxburgh, I. W., Samadi, R., Steslicki, M., Uytterhoeven, K., Verner, G. A., Auvergne, M., Baglin, A., Forteza, S. Barcelo, Baudin, F., Cortes, T. Roca |
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| Rok vydání: | 2013 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| Popis: | The satellite CoRoT (Convection, Rotation, and planetary Transits) has provided high-quality data for almost six years. We show here the asteroseismic analysis and modeling of HD169392A, which belongs to a binary system weakly gravitationally bound as the distance between the two components is of 4250 AU. The main component, HD169392A, is a G0IV star with a magnitude of 7.50 while the second component is a G0V-G2IV star with a magnitude of 8.98. This analysis focuses on the main component, as the secondary one is too faint to measure any seismic parameters. A complete modeling has been possible thanks to the complementary spectroscopic observations from HARPS, providing Teff=5985+/-60K, log g=3.96+/-0.07, and [Fe/H]=- 0.04+/-0.10. Comment: 6 pages, 1 figure. Proceedings of the Fujihara seminar held in Hakone (Japan) in November 2012 |
| Databáze: | arXiv |
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