The nature of cold gas in the Chamaeleon molecular cloud complex
The gas content of the Milky Way has been typically studied through observations of carbon monoxide (CO) and neutral atomic hydrogen (H i) spectral lines. However, when we compare the column density measurements from these data sets with those from gamma ray observations, we find an apparent discrep...
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| Autor principal: | |
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| Formato: | bachelorThesis |
| Publicado em: |
2025
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| Acesso em linha: | https://repositorio.yachaytech.edu.ec/handle/123456789/1028 |
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