ALMACAL – VI. Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
We are just starting to understand the physical processes driving the dramatic change in cosmic star formation rate between z ∼ 2 and the present day. A quantity directly linked to star formation is the molecular gas density, which should be measured through independent methods to explore variations...
| المؤلفون الرئيسيون: | , , , , , , , , , , , , , , |
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| التنسيق: | Journal article |
| اللغة: | English |
| منشور في: |
Oxford University Press
2019
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