The Lambda Orionis Star Forming Region: the Spitzer perspective
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| Format: | Artículo científico |
| Sprache: | en |
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Universidad Nacional Autónoma de México
2007
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| _version_ | 1876487329203355648 |
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| author | D. Barrado y Navascués |
| author_facet | D. Barrado y Navascués |
| contents | The Lambda Orionis Star Forming Region: the Spitzer perspective D. Barrado y Navascués J. R. Stauffer M. Morales-Calderón A. Bayo Física, Astronomía y Matemáticas STARS: PRE H II REGIONS MAIN SEQUENCE STARS: MASS LOSS ISM: JETS AND OUTFLOWS The Head of Orion is a complex star forming region which includes a young open cluster (Collinder 69, about5 Myr), two dark clouds (Barnard 30 and Barnard 35, with younger populations) and other younger areas(LDN1588 and LDN1603). We have observed one square degree in each of these regions with Spitzer in orderto study the stellar and substellar population. These data have been complemented with optical and nearinfrared photometry and spectroscopy. We have studied the Class I and II relative population and tried tounderstand it in the context of the differences in the local environment and the evolution. 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102909 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.29 |
| format | Artículo científico |
| id | redalyc_57102909 |
| institution | Redalyc |
| language | en |
| publishDate | 2007 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | The Lambda Orionis Star Forming Region: the Spitzer perspective D. Barrado y Navascués Física, Astronomía y Matemáticas STARS: PRE H II REGIONS MAIN SEQUENCE STARS: MASS LOSS ISM: JETS AND OUTFLOWS The Lambda Orionis Star Forming Region: the Spitzer perspective D. Barrado y Navascués J. R. Stauffer M. Morales-Calderón A. Bayo Física, Astronomía y Matemáticas STARS: PRE H II REGIONS MAIN SEQUENCE STARS: MASS LOSS ISM: JETS AND OUTFLOWS The Head of Orion is a complex star forming region which includes a young open cluster (Collinder 69, about5 Myr), two dark clouds (Barnard 30 and Barnard 35, with younger populations) and other younger areas(LDN1588 and LDN1603). We have observed one square degree in each of these regions with Spitzer in orderto study the stellar and substellar population. These data have been complemented with optical and nearinfrared photometry and spectroscopy. We have studied the Class I and II relative population and tried tounderstand it in the context of the differences in the local environment and the evolution. 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102909 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.29 |
| title | The Lambda Orionis Star Forming Region: the Spitzer perspective |
| topic | Física, Astronomía y Matemáticas STARS: PRE H II REGIONS MAIN SEQUENCE STARS: MASS LOSS ISM: JETS AND OUTFLOWS |
| url | https://www.redalyc.org/articulo.oa?id=57102909 |