Exploring star formation in high-z galaxies using atomic and molecular emission lines
vor 10 Jahren
Beschreibung
vor 10 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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