Dust temperature maps of the Galactic plane: The Herschel spectral energy distribution fitting with Cloudy predictions
文献类型：期刊论文
| 作者 | Zhu, Jiali1,2 ; Huang, Maohai1
|
| 刊名 | ASTRONOMY & ASTROPHYSICS
 |
| 出版日期 | 2014-04-01 |
| 卷号 | 564 |
| 关键词 | ISM: general dust, extinction infrared: ISM methods: data analysis |
| 英文摘要 | Context. Dust grains absorb the interstellar far ultra-violet and visible photons and re-emit them in far-infrared (FIR) wavebands. The dust FIR continuum can be predicted by a grid of models using various values of the interstellar radiation field. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000334671000111 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6408]  |
| 专题 | 国家天文台_空间科学研究部 |
| 作者单位 | 1.Natl Astron Observ, Beijing 100012, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China |
| 推荐引用方式 GB/T 7714 | Zhu, Jiali,Huang, Maohai. Dust temperature maps of the Galactic plane: The Herschel spectral energy distribution fitting with Cloudy predictions[J]. ASTRONOMY & ASTROPHYSICS,2014,564. |
| APA | Zhu, Jiali,&Huang, Maohai.(2014).Dust temperature maps of the Galactic plane: The Herschel spectral energy distribution fitting with Cloudy predictions.ASTRONOMY & ASTROPHYSICS,564. |
| MLA | Zhu, Jiali,et al."Dust temperature maps of the Galactic plane: The Herschel spectral energy distribution fitting with Cloudy predictions".ASTRONOMY & ASTROPHYSICS 564(2014). |
入库方式： OAI收割
来源：国家天文台
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