THE INNER GALACTIC STRUCTURE TRACED BY MOLECULAR CLOUDS ASSOCIATED WITH ULTRA-COMPACT HII REGIONS
We are testing a method to solve for the distances of a sample of ultra-compact (UC) HII regions with IRAS colors and CS(J=2-1) detection. The ambiguity in their kinematical distances is solved using Monte-Carlo simulations. We simulated heliocentric longitude-Radius (l-R) on Galactic plane distribu...
Сохранить в:
| Опубликовано в:: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Главные авторы: | , , |
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
Universidad Nacional Autónoma de México
2008
|
| Предметы: | |
| Online-ссылка: | https://www.redalyc.org/articulo.oa?id=57116170033 |
| Метки: |
Нет меток, Требуется 1-ая метка записи!
|
