Abstract
Long slit spectra at high S/N of a sample of Giant Extragalactic H II Regions and H II galaxies, show evidence for very high velocity ionized gas. This kind of phenomenon appears to be localized in a limited area within the observed regions. The most peculiar object in the sample is NGC 2363, where the profiles of the emission lines detected in the nuclear zone suggest non-symmetrical motions.
| Original language | English |
|---|---|
| Pages (from-to) | 113-116 |
| Number of pages | 4 |
| Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
| Volume | 3 |
| State | Published - 1995 |
| Externally published | Yes |
| Event | 5th Mexico-Texas Conference on Astrophysics: Gaseous Nebulae and Star Formation - Tequesquitengo, Mor, Mexico Duration: 3 Apr 1995 → 5 Apr 1995 |
Keywords
- H II regions
- ISM: kinematics and dynamics