The chemistry of stellar Jets
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| Formato: | Artículo científico |
| Lenguaje: | en |
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Universidad Nacional Autónoma de México
2002
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| _version_ | 1876454012996288512 |
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| author | D. A. Williams |
| author_facet | D. A. Williams |
| contents | The chemistry of stellar Jets D. A. Williams A. J. Lim S. Viti Física, Astronomía y Matemáticas ISM: SHOCKS ISM: CHEMISTRY ISM: MOLECULAR CLOUDS STARS: JETS AND OUTFLOWS Many astronomical phenomena are conveniently explored through observations of molecular line emission. Inthis paper, we discuss the chemistry that gives rise to molecular tracers in two scenarios associated with theinteraction of stellar jets with molecular clouds. The rst situation is the environment of the bow shock nearthe head of a jet entering a molecular cloud. The second is the case of a clump within a molecular cloud thatis a ected by the intense radiation eld generated in the jet/cloud shock. In both cases, specic moleculartracers of the physical conditions can be identied. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101322 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.13 |
| format | Artículo científico |
| id | redalyc_57101322 |
| institution | Redalyc |
| language | en |
| publishDate | 2002 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | The chemistry of stellar Jets D. A. Williams Física, Astronomía y Matemáticas ISM: SHOCKS ISM: CHEMISTRY ISM: MOLECULAR CLOUDS STARS: JETS AND OUTFLOWS The chemistry of stellar Jets D. A. Williams A. J. Lim S. Viti Física, Astronomía y Matemáticas ISM: SHOCKS ISM: CHEMISTRY ISM: MOLECULAR CLOUDS STARS: JETS AND OUTFLOWS Many astronomical phenomena are conveniently explored through observations of molecular line emission. Inthis paper, we discuss the chemistry that gives rise to molecular tracers in two scenarios associated with theinteraction of stellar jets with molecular clouds. The rst situation is the environment of the bow shock nearthe head of a jet entering a molecular cloud. The second is the case of a clump within a molecular cloud thatis a ected by the intense radiation eld generated in the jet/cloud shock. In both cases, specic moleculartracers of the physical conditions can be identied. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101322 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.13 |
| title | The chemistry of stellar Jets |
| topic | Física, Astronomía y Matemáticas ISM: SHOCKS ISM: CHEMISTRY ISM: MOLECULAR CLOUDS STARS: JETS AND OUTFLOWS |
| url | https://www.redalyc.org/articulo.oa?id=57101322 |