Impact of internal gravity waves on the rotation profile inside pre-main sequence low-mass stars

Author： Charbonnel C.   Decressin T.   Amard L.   Palacios A.   Talon S.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|554|issue|A40-A40

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.554, Iss.issue, 2013-06, pp. : A40-A40

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Characterization of low-mass pre-main sequence stars in the Southern Cross

By  

Astronomy & Astrophysics, Vol. 384, Iss. 2, 2002-03 ,pp. : 521-531

Edp Sciences

Access to resources Recommend Favorite

New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit

By Baraffe Isabelle   Homeier Derek   Allard France   Chabrier Gilles  

Astronomy & Astrophysics, Vol. 577, Iss. issue, 2015-04 ,pp. : A42-A42

Edp Sciences

Access to resources Recommend Favorite

Low mass pre-main sequence stars in the Large Magellanic Cloud

By  

Astronomy & Astrophysics, Vol. 446, Iss. 3, 2006-02 ,pp. : 955-969

Edp Sciences

Access to resources Recommend Favorite

Combined effects of tidal and rotational distortions on the equilibrium configuration of low-mass, pre-main sequence stars

By  

Astronomy & Astrophysics, Vol. 494, Iss. 1, 2009-01 ,pp. : 209-227

Edp Sciences

Access to resources Recommend Favorite

New low-mass pre-main sequence spectroscopic binaries in Orion

By  

Astronomy & Astrophysics, Vol. 375, Iss. 1, 2001-08 ,pp. : 130-144

Edp Sciences

Access to resources Recommend Favorite