Skip to main content Accessibility help
×
Home

Angular Momentum Evolution of Young Solar-type Stars

  • Louis Amard (a1) (a2), Ana Palacios (a1) and Corinne Charbonnel (a2) (a3)

Abstract

We present stellar evolution models of young solar-type stars including self consistent treatment of rotational mixing and extraction of angular momentum (AM) by magnetized wind including the most up-to-date physic of AM transport.

    • Send article to Kindle

      To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

      Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

      Find out more about the Kindle Personal Document Service.

      Angular Momentum Evolution of Young Solar-type Stars
      Available formats
      ×

      Send article to Dropbox

      To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

      Angular Momentum Evolution of Young Solar-type Stars
      Available formats
      ×

      Send article to Google Drive

      To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

      Angular Momentum Evolution of Young Solar-type Stars
      Available formats
      ×

Copyright

References

Hide All
Amard, L., Palacios, A., Charbonnel, C. in prep
Bouvier, J. 2008, A&A, 489, 53
Charbonnel, C., Decressin, T., Amard, L., Palacios, A., & Talon, S. 2013, A&A, 554, A40
Charbonnel, C. & Talon, S. 2005, Science, 309, 2189
Eggenberger, P., Maeder, A., & Meynet, G. 2005, A&A, 440, L9
Endal, A. S. & Sofia, S. 1976, ApJ, 210, 184
Gallet, F. & Bouvier, J. 2013, A&A, 556, A36
Gallet, F. & Bouvier, J. 2015, A&A, 577, A98
García, R.-A., Salabert, D., & Ballot, J.et al. 2011, JPhCS, 271
Krishna-Swamy, K. S. 1966, ApJ 145, 174
Lagarde, N. & Decressin, T., Charbonnel, C.et al. 2012, A&A, 543, 108
Maeder, A. & Zahn, J.-P. 1998, A&A, 334, 1000
Mathis, S., Palacios, A., & Zahn, J.-P. 2004, A&A, 425, 243
Mathis, S. & Zahn, J.-P. 2004, A&A, 425, 229
Matt, S., Brun, A. S., Baraffe, I., Bouvier, J., & Chabrier, G. 2015, ApJ, 799, L23
McQuillan, A., Mazeh, T., & Aigrain, S. 2013, ApJL, 775, L11
Palacios, A., Charbonnel, C., Talon, S., & Siess, L. 2006, A&A, 453, 261
Siess, L., Dufour, E., & Forestini, M. 2000, A&A, 358, 593
Talon, S. & Zahn, J.-P. 1997, A&A, 317, 749
Vandenberg, D. A., Edvardsson, B., Eriksson, K., Gustafsson, B., & Ferguson, J. W. 2007, in IAU Symp. 241, Stellar Populations as Building Blocks of Galaxies, p. 23
Zahn, J.-P. 1992, A&A, 265, 115
MathJax
MathJax is a JavaScript display engine for mathematics. For more information see http://www.mathjax.org.

Keywords

Angular Momentum Evolution of Young Solar-type Stars

  • Louis Amard (a1) (a2), Ana Palacios (a1) and Corinne Charbonnel (a2) (a3)

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed