Exploring star formation in high-z galaxies using atomic and molecular emission lines

The conditions under which stars are formed and the reasons for triggering and quenching of starburst events in high-z galaxies, are still not well understood. Studying the interstellar medium (ISM) and the morphology of high-z galaxies are therefore key points in order to understand galaxy evolution. The cosmic star formation rate density peaks between 1 >1, and low to moderate [CII] optical depth tau(CII) 2, pave the road for future investigations of the star-forming ISM in high-z galaxies, by illustrating the importance of multi-wavelength, fine structure- and molecular line studies.

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Exploring star formation in high-z galaxies using atomic and molecular emission lines is an episode from Fakultät für Physik - Digitale Hochschulschriften der LMU - Teil 05/05 by Ludwig-Maximilians-Universität München.

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This episode was published on Mar 14, 2016.

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