Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars

Publisher： Edp Sciences

E-ISSN： 1432-0746|508|1|409-419

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.508, Iss.1, 2009-12, pp. : 409-419

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

Pulsational instabilities driven by the ∈ mechanism in hot pre-horizontal branch stars

By Battich Tiara   Bertolami Marcelo M. Miller   Córsico Alejandro H.   Althaus Leandro G.  

Astronomy & Astrophysics, Vol. 614, Iss. issue, 2018-07 ,pp. : A136-A136

Edp Sciences

Access to resources Recommend Favorite

Gravity modes in rapidly rotating stars

By Ballot J.   Lignières F.   Reese D. R.   Rieutord M.  

Astronomy & Astrophysics, Vol. 518, Iss. issue, 2010-08 ,pp. : A30-A30

Edp Sciences

Access to resources Recommend Favorite

The winds of hot massive first stars

By  

Astronomy & Astrophysics, Vol. 446, Iss. 3, 2006-02 ,pp. : 1039-1049

Edp Sciences

Access to resources Recommend Favorite

Magnetic spots on hot massive stars

By Cantiello M.   Braithwaite J.  

Astronomy & Astrophysics, Vol. 534, Iss. issue, 2011-10 ,pp. : A140-A140

Edp Sciences

Access to resources Recommend Favorite

Temperature and gravity scales in hot stars

By  

EAS Publications Series, Vol. 64, Iss. issue, 2014-02 ,pp. : 47-54

Edp Sciences

Access to resources Recommend Favorite