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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...

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Bibliografski detalji
Izdano u:Revista Mexicana de Astronomía y Astrofísica
Glavni autori: A. Luna, M. L. Ortega, E. de la Fuente
Format: Artigo
Jezik:Inglês
Izdano: Universidad Nacional Autónoma de México 2008
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Online pristup:https://www.redalyc.org/articulo.oa?id=57116170033
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