“PAH”的版本间差异
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无编辑摘要 |
无编辑摘要 |
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*PAHs are better suited as a tracer of B stars than as a tracer of massive SF. They probe star formation activity time scales of up to 100Myr. [http://astro.dur.ac.uk/AGNvsSF/Talks/AlonsoHerrero.pdf] |
*PAHs are better suited as a tracer of B stars than as a tracer of massive SF. They probe star formation activity time scales of up to 100Myr. [http://astro.dur.ac.uk/AGNvsSF/Talks/AlonsoHerrero.pdf] |
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*Mapping RPAH across the 19 [[PHANGS]] galaxies, we find that the PAH fraction steeply decreases in HII regions, revealing the destruction of these small grains in regions of ionized gas. Outside HII regions, we find RPAH is constant across the PHANGS sample with an average value of 3.43±0.98, which, for an illuminating radiation field of intensity 2-5 times that of the radiation field in the solar neighborhood, corresponds to qPAH values of 3-6%. arXiv:2405.15102 |
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*[[PAHFIT]] |
*[[PAHFIT]] |
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2024年5月27日 (一) 07:04的版本
- PAH 的辐射
- 3.3um C-H键震动，脂肪族的C-H键震动在3.4um
- 6.2,7.6um是C-C拉伸震动
- 7.8,8.6 C-H在平面内弯曲，11.3,12.7平面外弯曲
- 17um,C-C-C弯曲，18mu有硅的发射特征
- PAHs are better suited as a tracer of B stars than as a tracer of massive SF. They probe star formation activity time scales of up to 100Myr. [1]
- Mapping RPAH across the 19 PHANGS galaxies, we find that the PAH fraction steeply decreases in HII regions, revealing the destruction of these small grains in regions of ionized gas. Outside HII regions, we find RPAH is constant across the PHANGS sample with an average value of 3.43±0.98, which, for an illuminating radiation field of intensity 2-5 times that of the radiation field in the solar neighborhood, corresponds to qPAH values of 3-6%. arXiv:2405.15102