New Theory of Stellar Convection without the mixing-length parameter: new stellar atmosphere models

Publisher： Cambridge University Press

E-ISSN： 1743-9221|11|A29B|154-155

ISSN： 1743-9213

Source： Proceedings of the International Astronomical Union, Vol.11, Iss.A29B, 2016-10, pp. : 154-155

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

Theory of stellar convection: removing the mixing-length parameter

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 608-613

Cambridge University Press

Access to resources Recommend Favorite

Stellar yields – theory and observations

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 162-163

Cambridge University Press

Access to resources Recommend Favorite

New PARSEC database of alpha enhanced stellar evolutionary tracks and isochrones for Gaia

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 144-146

Cambridge University Press

Access to resources Recommend Favorite

Probing the Martian atmosphere with MAVEN/IUVS stellar occultations

By  

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9064-9070

John Wiley & Sons Inc

Access to resources Recommend Favorite

Mixing‐length controls on high‐resolution simulations of convective storms

By  

THE QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol. 141, Iss. 686, 2015-01 ,pp. : 272-284

John Wiley & Sons Inc

Access to resources Recommend Favorite