In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 163 ( 1995), p. 154-155
Abstract:
We present an analysis of high resolution UV ( IUE ) and optical ( INT, AAT and ESO ) spectroscopy of eight galactic WN and WC stars. We examine the correlation between ionization potential (IP) and the velocity structure of the stellar winds and find important correlations between line-width, IP and excitation potential (EP). These results provide potential constraints on the velocity law used in models of WR atmospheres.
Type of Medium:
Online Resource
ISSN:
0074-1809
DOI:
10.1017/S0074180900201824
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1995
SSG:
16,12