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Structure and dynamics of high-z galaxies

Published online by Cambridge University Press:  14 May 2020

Stijn Wuyts Open the ORCID record for Stijn Wuyts [Opens in a new window]  and
Natascha M. Förster Schreiber
Stijn Wuyts
Affiliation:
Dept. of Physics, University of Bath, Claverton Down, Bath, BA2 7AY, UK email: s.wuyts@bath.ac.uk
Natascha M. Förster Schreiber
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, Garching, D-85737, Germany email: forster@mpe.mpg.de
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Abstract

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HST and integral-field spectroscopic observations of star-forming galaxies at cosmic noon provide a view on the spatial distribution of stars, gas and dust, and probe gaseous motions revealing the central gravitational potential and local feedback processes at play. In this paper, we review recent insights gained from such observations, with an emphasis on results obtained through near-infrared imaging spectroscopy. Their context and implications are documented more fully in a forthcoming review article by Förster Schreiber & Wuyts (in prep).

Keywords

Galaxies: structureGalaxies: kinematicsGalaxies: high-redshift
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 271 - 278
Copyright
© International Astronomical Union 2020

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