OH AND CN ZEEMAN OBSERVATIONS OF MAGNETIC FIELDS IN MOLECULAR CLOUDS
Observations of the Zeeman e ect in OH and CN provide valuable information about magnetic eld strengths and directions in molecular clouds in the density range 103 < n(cm-3) < 106 that these species sample. These data make it possible to test predictions of weak eld, turbulence driven star formation...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2009
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57115743016 |
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