The effects of rotation and stellar magnetic fields on the nebular shapes: LBV nebulae and PNe

G. Garcia-Segura1, N. Langer2, M. Rozyczka3, M.-M. Mac Low4, J. Franco4

1Instituto de Astronomia-UNAM, Mexico
2Institut für Theoretische Physik und Astrophysik, Universität Potsdam
3Warsaw University Observatory, Warszawa, Poland
4also N. Copernicus Astronomical Center, Warszawa, Poland
5Max-Planck-Institut für Astronomie, Heidelberg,

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/nlanger/texmex.ps (127kB uncompressed) or texmex.ps.gz (49kB compressed).

Display full article with ghostview (local users only!)

Fetch PostScript-File (texmex.ps, 127kB, uncompressed)

Fetch PostScript-File (texmex.ps.gz, 49kB, compressed)

Zurück zur Übersicht