Morpho-Kinematic Modeling of Gaseous Nebulae with SHAPE
We present a powerful new tool to analyse and disentangle the 3-D geometryand kinematic structure of gaseous nebulae. The method consists in combiningcommercially available digital animation software to simulate the 3-D structure andexpansion pattern of the nebula with a dedicated, purpose-built ren...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2006
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57142110 |
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