Stellar Midlife Crises: Challenges and Advances in Simulating Convection and Differential Rotation in Sun-like Stars

E-ISSN： 1743-9221|12|S328|264-273

ISSN： 1743-9213

Source： Proceedings of the International Astronomical Union, Vol.12, Iss.S328, 2017-09, pp. : 264-273

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

Improved rotation-activity-age relations in Sun-like stars

Proceedings of the International Astronomical Union, Vol. 12, Iss. S328, 2017-09 ,pp. : 274-281

Cambridge University Press

Access to resources Recommend Favorite

Differential rotation of stars with multiple transiting planets

Proceedings of the International Astronomical Union, Vol. 12, Iss. S328, 2017-09 ,pp. : 107-109

Cambridge University Press

Access to resources Recommend Favorite

Pulsations in hot subdwarf stars: recent advances and prospects for testing stellar physics

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 581-588

Cambridge University Press

Access to resources Recommend Favorite

How to make the Sun look less like the Sun and more like a star?

Proceedings of the International Astronomical Union, Vol. 12, Iss. S328, 2017-09 ,pp. : 237-239

Cambridge University Press

Access to resources Recommend Favorite

Theory of stellar convection: removing the mixing-length parameter

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

Cambridge University Press

Access to resources Recommend Favorite