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REVEALING THE GALACTIC "UNDERGROUND" STAR FORMATION
We are reporting some recent results from our long-term program aimed at better understanding of the hidden present-day star cluster population in the Galaxy. So far, most clusters from our studies have typical ages of 3{10 Myr, and typical masses of order of a few thousand solar masses. Only two of...
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| Gepubliceerd in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hoofdauteurs: | , , |
| Formaat: | Artigo |
| Taal: | Espanhol |
| Gepubliceerd in: |
Universidad Nacional Autónoma de México
2009
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| Onderwerpen: | |
| Online toegang: | https://www.redalyc.org/articulo.oa?id=57115758017 |
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