Exploring star formation in high-z galaxies using atomic and molecular emission lines
Beschreibung
vor 8 Jahren
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.
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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