Abstract
We present new spectroscopic data on the three most pronounced H II regions in IC 4662, where the metal content is obtained from the electronic temperature method. Two of these, named regions A1 and A2, present the same chemical abundances for all the elements studied, but the third one, named D, has very discordant abundances.
| Original language | English |
|---|---|
| Pages (from-to) | 242-243 |
| Number of pages | 2 |
| Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
| Volume | 12 |
| State | Published - 2002 |
| Externally published | Yes |
| Event | Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert - Mexico City, Mexico Duration: 21 Nov 2000 → 24 Nov 2000 |
Keywords
- Galaxies: dwarf
- Galaxies: irregular
- ISM: abundances