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Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

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Silva Aguirre,  Victor
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Bedding, T. R., Mosser, B., Huber, D., Montalbán, J., Beck, P., Christensen-Dalsgaard, J., Elsworth, Y. P., García, R. A., Miglio, A., Stello, D., White, T. R., De Ridder, J., Hekker, S., Aerts, C., Barban, C., Belkacem, K., Broomhall, A.-M., Brown, T. M., Buzasi, D. L., Carrier, F., Chaplin, W. J., Di Mauro, M. P., Dupret, M.-A., Frandsen, S., Gilliland, R. L., Goupil, M.-J., Jenkins, J. M., Kallinger, T., Kawaler, S., Kjeldsen, H., Mathur, S., Noels, A., Silva Aguirre, V., & Ventura, P. (2011). Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars. Nature, 471(7340), 608-611. doi:10.1038/nature09935.


引用: https://hdl.handle.net/11858/00-001M-0000-0011-5435-3
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