Determining the Composition of Dust Formed in Quasar Winds
碩士 === 國立臺灣師範大學 === 物理學系 === 101 === Forming dust is difficult, it needs a high density and low temperature (<2000K) environment. Therefore, where the dust in the torus around Active Galactic Nuclei (AGN) comes from is an interesting question. It could be processed interstellar dust, or, as Elvis e...
| Main Authors: | , |
|---|---|
| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2013
|
| Online Access: | http://ndltd.ncl.edu.tw/handle/17431814205975817163 |