Structure and dynamics of high-z galaxies

Stijn Wuyts; Natascha M. Förster Schreiber

doi:10.1017/S1743921319009293

Structure and dynamics of high-z galaxies

Stijn Wuyts, Natascha M. Förster Schreiber

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Abstract

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).

Original language	English
Pages (from-to)	271-278
Number of pages	8
Journal	Proceedings of the International Astronomical Union
Volume	14
Issue number	S353
Early online date	14 May 2020
DOIs	https://doi.org/10.1017/S1743921319009293
Publication status	Published - 30 Jun 2020

Bibliographical note

Publisher Copyright:
© 2020 International Astronomical Union.

Keywords

Galaxies: high-redshift
Galaxies: kinematics
Galaxies: structure

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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Cite this

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Structure and dynamics of high-z galaxies

Abstract

Bibliographical note

Keywords

ASJC Scopus subject areas

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