Aquecimento em colunas de acreção de estrelas T Tauri
=== Young low mass stars that show signs of accretion, the classical T Tauri stars (CTTSs), present a significant number of emission lines in their spectra. These emission lines, thought to be produced in accretion columns, are often modelled in order to obtain physical parametersof the star-disk s...
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| Format: | Others |
| Language: | Portuguese |
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Universidade Federal de Minas Gerais
2011
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| Online Access: | http://hdl.handle.net/1843/JCBV-8PBHRJ |