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[//]: # ( ## The Cloudy spectral synthesis code)
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[//]: # ( ## The Cloudy spectral synthesis code)
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----
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![Cloudy produced spectrum of the Perseus model with log column density 24, showing resolved fine-structure doublets, with a spectral resolution of R = 0.25 eV.](uploads/f5b76a659760edd4dc97ca97f48a7e0f/Figure_1_2.png)
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![](uploads/f5b76a659760edd4dc97ca97f48a7e0f/Figure_1_2.png)
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*Cloudy produced spectrum of a model of the environment in the outer region of
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Perseus core. The figure shows resolved fine-structure doublets, using a spectral resolution of R = 0.25 eV. The model has a log column density of 24.*
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----
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Cloudy is a spectral synthesis code designed to simulate conditions in interstellar matter under a broad range of conditions. It is provided for general use under an open-source
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Cloudy is a spectral synthesis code designed to simulate conditions in interstellar matter under a broad range of conditions. It is provided for general use under an open-source
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[License](License).
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[License](License).
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