Fabry-Perot Observations of HH 1/2
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| Format: | Artículo científico |
| Language: | en |
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Universidad Nacional Autónoma de México
2005
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| _version_ | 1876468125014163456 |
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| author | Ph. Amram |
| author_facet | Ph. Amram |
| contents | Fabry-Perot Observations of HH 1/2 Ph. Amram J. Boulesteix O. Toledano A. Riera A. C. Raga B. Reipurth Física, Astronomía y Matemáticas HH 2) ISM: HERBIG HARO OBJECTS ISM: INDIVIDUAL (HH 1 ISM: JETS AND OUTFLOWS We present new H Fabry-Perot observations of the HH 1/2 system. Lineprofiles, barycenter radial velocity maps and dispersion maps are derived from thechannel maps of HH 1 and HH 2. The radial velocity barycenter maps of both HH 1and HH 2 show a general trend of \red-shifted upstream/blue-shifted downstream"pattern. A \direct+scattered" component model for three emitting condensationsis qualitatively successful at reproducing the general features of the barycenter andthe velocity dispersion of HH 2. 2005 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57141201 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) Num.2 Vol.41 |
| format | Artículo científico |
| id | redalyc_57141201 |
| institution | Redalyc |
| language | en |
| publishDate | 2005 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Fabry-Perot Observations of HH 1/2 Ph. Amram Física, Astronomía y Matemáticas HH 2) ISM: HERBIG HARO OBJECTS ISM: INDIVIDUAL (HH 1 ISM: JETS AND OUTFLOWS Fabry-Perot Observations of HH 1/2 Ph. Amram J. Boulesteix O. Toledano A. Riera A. C. Raga B. Reipurth Física, Astronomía y Matemáticas HH 2) ISM: HERBIG HARO OBJECTS ISM: INDIVIDUAL (HH 1 ISM: JETS AND OUTFLOWS We present new H Fabry-Perot observations of the HH 1/2 system. Lineprofiles, barycenter radial velocity maps and dispersion maps are derived from thechannel maps of HH 1 and HH 2. The radial velocity barycenter maps of both HH 1and HH 2 show a general trend of \red-shifted upstream/blue-shifted downstream"pattern. A \direct+scattered" component model for three emitting condensationsis qualitatively successful at reproducing the general features of the barycenter andthe velocity dispersion of HH 2. 2005 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57141201 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) Num.2 Vol.41 |
| title | Fabry-Perot Observations of HH 1/2 |
| topic | Física, Astronomía y Matemáticas HH 2) ISM: HERBIG HARO OBJECTS ISM: INDIVIDUAL (HH 1 ISM: JETS AND OUTFLOWS |
| url | https://www.redalyc.org/articulo.oa?id=57141201 |