Observational indicators of the transition from fully convective stars to stars with radiative cores

Author： Mayne N. J.  

Publisher： Oxford University Press

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.408, Iss.3, 2010-11, pp. : 1409-1416

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

Differential rotation in fully convective stars

By Balbus Steven A.   Weiss Nigel O.  

Monthly Notices of the Royal Astronomical Society, Vol. 404, Iss. 3, 2010-05 ,pp. : 1263-1271

Oxford University Press

Access to resources Recommend Favorite

FROM CORES TO STARS

By  

Astrophysics and Space Science, Vol. 292, Iss. 1-4, 2004-08 ,pp. : 291-291

Springer Publishing Company

Access to resources Recommend Favorite

Modelling fully convective stars in eclipsing binaries: KOI-126 and CM Draconis

By Spada F.   Demarque P.  

Monthly Notices of the Royal Astronomical Society, Vol. 422, Iss. 3, 2012-05 ,pp. : 2255-2261

Oxford University Press

Access to resources Recommend Favorite

From Cores to Stars, Brown Dwarfs and Planets

By Rebolo Rafael  

Astrophysics and Space Science, Vol. 292, Iss. 1-4, 2004-08 ,pp. : 293-295

Springer Publishing Company

Access to resources Recommend Favorite

From Molecular Cores to Stars and Brown Dwarfs

By Bate Matthew  

Astrophysics and Space Science, Vol. 292, Iss. 1-4, 2004-08 ,pp. : 297-307

Springer Publishing Company

Access to resources Recommend Favorite