Author： Sundqvist J. O. Puls J. Feldmeier A.
Publisher： Edp Sciences
E-ISSN： 1432-0746|510|issue|A11-A11
ISSN： 0004-6361
Source： Astronomy & Astrophysics, Vol.510, Iss.issue, 2010-01, pp. : A11-A11
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
Mass loss from inhomogeneous hot star winds
By Sundqvist J. O. Puls J. Feldmeier A. Owocki S. P.
Astronomy & Astrophysics, Vol. 528, Iss. issue, 2011-03 ,pp. :
Access to resources
Recommend
Mass loss from inhomogeneous hot star winds
By Sundqvist J. O. Puls J. Owocki S. P.
Astronomy & Astrophysics, Vol. 568, Iss. issue, 2014-08 ,pp. :
Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates
Astronomy & Astrophysics, Vol. 476, Iss. 3, 2007-12 ,pp. :
On the wavelength drift of spectral features from structured hot star winds
Astronomy & Astrophysics, Vol. 378, Iss. 3, 2001-11 ,pp. :
Structure and dynamics of hot star winds
EAS Publications Series, Vol. 13, Iss. issue, 2010-03 ,pp. :