A publishing partnership

The Propagation of Kinks in Line-driven Winds

, , and

© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation A. Feldmeier et al 2008 ApJ 679 704 DOI 10.1086/587616

0004-637X/679/1/704

Abstract

We show that discontinuities in spatial derivatives of the velocity and density law, so-called kinks, can propagate upstream at Mach numbers > 1 with respect to radiative-acoustic waves in stellar winds driven by radiation scattering in spectral lines. This fast upstream propagation of kinks can, for example, explain the slow evolution of discrete absorption components found in P Cygni line profiles from O stars.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/587616