查看“HII region”的源代码

*PHANGS-MUSE survey
*PHANGS-JWST
:4个星系：Two galaxies (NGC 1365 and NGC 7496) host active galactic nuclei (AGNs) and strong bars. NGC 628 is a prototypical grand-design spiral, while IC 5332 shows a flocculent spiral morphology. Based on MUSE Hα emission line maps, a catalog of ∼ 30, 000 nebulae has been constructed. The nebulae were selected using HIIphot.

:arXiv:2212.09159: 利用JWST/MIRI images in the F770W, F1000W and F1130W来计算q(PAH)=(F770+F1130)/F2100来计算PAH在尘埃中的比例，F2100是用来表示非常小的尘埃颗粒的发射，从而代表总尘埃。SIII/SII表征电离参数，发现q(PAH)最主要和电离参数相关，而和金属丰度关系不大
* HII区和分子云区域的转换非常的sharp  [https://arxiv.org/pdf/2307.09513.pdf]

*利用IFS数据来搜寻HII区的软件 pyHIIexplorer [https://github.com/cespinosa/pyHIIexplorerV2] arXiv:2204.04252
*利用发射线来算金属丰度
:*[[HII-CHI-MISTRY]]
:*GAME （机器学习的方法）https://arxiv.org/abs/1803.10236
:*  nebulabayes: [https://pypi.org/project/NebulaBayes/]
:* HIIlines [https://github.com/Sheng-Qi-Yang/HIILines]