TY  - JOUR
A1  - Gräfener, Götz
A1  - Koesterke, Lars
A1  - Hamann, Wolf-Rainer
T1  - The WR population in CTS 1026
N2  - The blue compact H II galaxy CTS 1026 shows very strong WR emission features around 4686 AA and 5800 AA. We present high S/N optical spectra of the nucleus of this object. Byanalysis of the WR profile shapes, we determine the dominant spectral types and the WN/WC ratio in the starforming region. The ratio WR/O is determined via standard nebular diagnostics.
Y1  - 2003
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/15769
SN  - 1-58381-133-8
ER  -