The AG Carinae nebula revisited.
Abstract
We report new Cassegrain observation of the AG Car nebula, as well as long slit Coude spectra and imagery at H-alpha. From our data we derive an expansion velocity of 66 km/s for the nebula and a minimal mass of 2.7 solar mass. Long slit data show H-alpha emission up to 45 arcsec from the star, indicating a diffuse nebulosity surrounding the main nebula. We also find that nitrogen is overabundant by one order of magnitude and oxygen is deficient at least by a factor of 6 in the nebula. These results are consistent with the surface abundances of a 60 solar mass star aged at 3.7 x 10 exp 6 yr just beginning its LBV phase.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- December 1992
- Bibcode:
- 1992A&A...266..360D
- Keywords:
-
- Nebulae;
- Stellar Envelopes;
- Stellar Evolution;
- Stellar Mass Ejection;
- Abundance;
- Cassegrain Optics;
- Emission Spectra;
- H Alpha Line;
- Stellar Composition;
- Stellar Models;
- Astrophysics