X-ray line profiles from structured stellar winds

L. Oskinova, W.-R. Hamann, A. Feldmeier

Universität Potsdam, Institut für Physik, Lehrstuhl Astrophysik
Postfach 601553, D-14415 Potsdam, Germany

Absorbing material compressed in a number of thin shells is effectively less opaque for X-rays than smoothly distributed gas. The calculated X-ray emission line profiles are red-shifted if the emission arises from the starward side of the shells.

The full article is available as PostScript file via anonymous ftp.
Server: ftp.astro.physik.uni-potsdam.de
user: anonymous or ftp; Password: your e-mail address;
file: pub/oskinova/lanzarote.ps (302kB uncompressed) or oskinova/lanzarote.ps.gz (77kB compressed).

Display full article with ghostview (local users only!)

Fetch PostScript-File (oskinova/lanzarote.ps, 302kB, uncompressed)

Fetch PostScript-File (oskinova/lanzarote.ps.gz, 77kB, compressed)

Zurück zur Übersicht