Light variations due to the line-driven wind instability and wind blanketing in O stars

Author： Krtička J.   Feldmeier A.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|617|issue|A121-A121

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.617, Iss.issue, 2018-09, pp. : A121-A121

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

2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach

By Sundqvist J. O.   Owocki S. P.   Puls J.  

Astronomy & Astrophysics, Vol. 611, Iss. issue, 2018-03 ,pp. : A17-A17

Edp Sciences

Access to resources Recommend Favorite

Instability of an accretion disk with a magnetically driven wind

By  

Astronomy & Astrophysics, Vol. 385, Iss. 1, 2002-04 ,pp. : 289-300

Edp Sciences

Access to resources Recommend Favorite

2D simulations of the line-driven instability in hot-star winds

By  

Astronomy & Astrophysics, Vol. 437, Iss. 2, 2005-07 ,pp. : 657-666

Edp Sciences

Access to resources Recommend Favorite

Two-dimensional simulations of the line-driven instability in hot-star winds

By  

Astronomy & Astrophysics, Vol. 406, Iss. 1, 2003-07 ,pp. : L1-L4

Edp Sciences

Access to resources Recommend Favorite

Maximum mass-loss rates of line-driven winds of massive stars

By  

Astronomy & Astrophysics, Vol. 403, Iss. 2, 2003-05 ,pp. : 625-635

Edp Sciences

Access to resources Recommend Favorite