Upper limit for the mass loss rate of rapidly rotating single main-sequence O9-B4 stars

ISSN： 1063-7737

Source： Astronomy Letters, Vol.36, Iss.11, 2010-11, pp. : 796-807

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

Related content

Population synthesis of rapidly rotating main-sequence stars with companions

By Raguzova N.

Astronomy Reports, Vol. 47, Iss. 5, 2003-05 ,pp. : 401-412

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Mass-loss in 2D zero-age main-sequence stellar models

By Lovekin C. C.

Monthly Notices of the Royal Astronomical Society, Vol. 415, Iss. 4, 2011-08 ,pp. : 3887-3894

Oxford University Press

Access to resources Recommend Favorite

Diffusion and Mixing in Main-Sequence Stars

By Vauclair S.

Astrophysics and Space Science, Vol. 284, Iss. 1, 2003-01 ,pp. : 205-215

Springer Publishing Company

Access to resources Recommend Favorite

Using 2MASS to detect main sequence companions to subdwarf B stars

By Reed M.D.

Astrophysics and Space Science, Vol. 291, Iss. 3-4, 2004-06 ,pp. : 329-332

Springer Publishing Company

Access to resources Recommend Favorite

Partial mixing of material in the radiative envelope and convective core of a rotating main-sequence star with mass 16M _⊙

By Staritsin E.

Astronomy Reports, Vol. 45, Iss. 6, 2001-06 ,pp. : 467-474

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite