The mass loss rates of Wolf-Rayet stars explained by optically thick radiation driven wind models

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@article{34b0f693e0e3424390b16bbb998a9081,

title = "The mass loss rates of Wolf-Rayet stars explained by optically thick radiation driven wind models",

author = "T. Nugis and H.J.G.L.M. Lamers",

year = "2002",

language = "Undefined/Unknown",

volume = "389",

pages = "162",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}