Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes-Reference-Cited by-同舟云学术

Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes

Published:2011-12-07 Issue:7379 Volume:481 Page:55-57
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Beck Paul G.,Montalban Josefina,Kallinger Thomas,De Ridder Joris,Aerts Conny,García Rafael A.,Hekker Saskia,Dupret Marc-Antoine,Mosser Benoit,Eggenberger Patrick,Stello Dennis,Elsworth Yvonne,Frandsen Søren,Carrier Fabien,Hillen Michel,Gruberbauer Michael,Christensen-Dalsgaard Jørgen,Miglio Andrea,Valentini Marica,Bedding Timothy R.,Kjeldsen Hans,Girouard Forrest R.,Hall Jennifer R.,Ibrahim Khadeejah A.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature10612.pdf

Reference24 articles.

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2. Sweigart, A. V. & Mengel, J. G. Meridional circulation and CNO anomalies in red giant stars. Astrophys. J. 229, 624–641 (1979)

3. Beck, P. G. et al. Kepler detected gravity-mode period spacings in a red giant star. Science 332, 205 (2011)

4. Bedding, T. R. et al. Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars. Nature 471, 608–611 (2011)

5. Zahn, J.-P. Circulation and turbulence in rotating stars. Astron. Astrophys. 265, 115–132 (1992)

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