Heavy mass loss from the symbiotic star AS 304.
Abstract
IUE, optical and infrared observations of the previously poorly studied symbiotic star AS 304 are discussed. The IUE low-resolution spectra are dominated by very strong P Cygni profiles of the resonant lines of N v, Si IV and C IV, indicating that the hot component of AS 304 is losing mass at a high rate via a fast wind. These P Cygni profiles make AS 304 almost unique among the symbiotic stars so far observed by the IUE. The hot component of AS 304 resembles the mass-losing nuclei of planetary nebulae.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- July 1993
- DOI:
- 10.1093/mnras/263.1.267
- Bibcode:
- 1993MNRAS.263..267M
- Keywords:
-
- Planetary Nebulae;
- Stellar Mass Ejection;
- Stellar Spectra;
- Symbiotic Stars;
- Astronomical Spectroscopy;
- Emission Spectra;
- Ionization;
- Iue;
- Spaceborne Astronomy;
- Astrophysics