ALMACAL – VI. Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers

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...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy:	Klitsch, A, Peroux, C, Zwaan, MA, Smail, I, Nelson, D, Popping, G, Chen, CC, Diemer, B, Ivison, RJ, Allison, JR, Muller, S, Swinbank, AM, Hamanowicz, A, Biggs, AD, Dutta, R
Format:	Journal article
Język:	English
Wydane:	Oxford University Press 2019

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