The physical conditions in SwSt 1 : the central star and the nebula.
Abstract
The authors present new optical observations on SwSt 1. They estimate a reddening of E(B-V) = 0.41 mag and a distance D = 1.2±0.2 kpc to the nebula. From their data the authors derive an electron density of (1.0±0.2)×105 cm-3 and a temperature of 11400±500K. Carbon, nitrogen, oxygen, chlorine and sulphur are underabundant more or less by a factor of 2 with respect to the "cosmic" values. The central star has an effective temperature of 32000K and is losing mass at a rate of (6 - 7)×10-8M_sun;yr-1.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- August 1987
- DOI:
- Bibcode:
- 1987MNRAS.227..773D
- Keywords:
-
- Late Stars;
- Planetary Nebulae;
- Carbon;
- Chlorine;
- Electron Density (Concentration);
- Nitrogen;
- Oxygen;
- Stellar Mass Ejection;
- Stellar Spectra;
- Stellar Temperature;
- Sulfur;
- Astrophysics