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Variable and Non-spherical Stellar Winds in Luminous Hot Stars
Tallenna

Variable and Non-spherical Stellar Winds in Luminous Hot Stars

There is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. The topics included OBA stars, Be stars, Wolf-Rayet stars, Be stars, and luminous blue variables (LBVs).
Alaotsikko
Proceedings of the IAU Colloquium No. 169 Held in Heidelberg, Germany, 15–19 June 1998
Painos
Softcover reprint of the original 1st ed. 1999
ISBN
9783662142103
Kieli
englanti
Paino
310 grammaa
Julkaisupäivä
23.8.2014
Sivumäärä
428