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| Format: | Artículo científico |
| Language: | en |
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Universidad Nacional Autónoma de México
2010
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| Online Access: | https://www.redalyc.org/articulo.oa?id=57115706024 |
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| _version_ | 1866558713986285568 |
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| author | S. Kraus |
| author_facet | S. Kraus |
| contents | INFRARED INTERFEROMETRY OF YOUNG STELLAR OBJECTS S. Kraus K.-H. Hofmann T. Preibisch G. Weigelt Física, Astronomía y Matemáticas outflows Accretion stars: pre stars: winds main sequence The circumstellar disks around young stellar objects play a key role in the formation process of stars and provide the stage for planet formation. Since recently, infrared interferometry provides the spatial resolution required to directly study the distribution of the gas and dust in the innermost AU around the forming star. We present recent investigations in which we employed the VLTI and its near- and mid-infrared interferometric instruments AMBER and MIDI to constrain the geometry and physical conditions of the disks around Herbig Ae/Be stars and to study the accretion and outflow processes taking place close to the central star. 2010 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115706024 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.38 |
| format | Artículo científico |
| id | redalyc_57115706024 |
| language | en |
| publishDate | 2010 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | INFRARED INTERFEROMETRY OF YOUNG STELLAR OBJECTS S. Kraus Física, Astronomía y Matemáticas outflows Accretion stars: pre stars: winds main sequence INFRARED INTERFEROMETRY OF YOUNG STELLAR OBJECTS S. Kraus K.-H. Hofmann T. Preibisch G. Weigelt Física, Astronomía y Matemáticas outflows Accretion stars: pre stars: winds main sequence The circumstellar disks around young stellar objects play a key role in the formation process of stars and provide the stage for planet formation. Since recently, infrared interferometry provides the spatial resolution required to directly study the distribution of the gas and dust in the innermost AU around the forming star. We present recent investigations in which we employed the VLTI and its near- and mid-infrared interferometric instruments AMBER and MIDI to constrain the geometry and physical conditions of the disks around Herbig Ae/Be stars and to study the accretion and outflow processes taking place close to the central star. 2010 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115706024 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.38 |
| title | INFRARED INTERFEROMETRY OF YOUNG STELLAR OBJECTS |
| topic | Física, Astronomía y Matemáticas outflows Accretion stars: pre stars: winds main sequence |
| url | https://www.redalyc.org/articulo.oa?id=57115706024 |