The WR population in CTS 1026
- 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.
| Author details: | Götz Gräfener, Lars Koesterke, Wolf-Rainer HamannORCiDGND |
|---|---|
| ISBN: | 1-58381-133-8 |
| Publication type: | Article |
| Language: | English |
| Year of first publication: | 2003 |
| Publication year: | 2003 |
| Release date: | 2017/03/24 |
| Source: | A massive star odyssey : from main sequence to supernova ; proceedings of the International Astronomical Union held in Costa Tequise / Hrsg.: Karl A. van der Hucht; Artemio Herrero; Cesar Esteban. - San Francisco : Astronomical Society of the Pacific, 2003. - ISBN: 1-58381-133-8. - S. 714 |
| Organizational units: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie |
| Institution name at the time of the publication: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik |
