Structure and dynamics of high-z galaxies

Stijn Wuyts, Natascha M. Förster Schreiber

Research output: Contribution to journalArticle

17 Downloads (Pure)

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 languageEnglish
Pages (from-to)271-278
Number of pages8
JournalProceedings of the International Astronomical Union
Volume14
Issue numberS353
Early online date14 May 2020
DOIs
Publication statusPublished - 30 Jun 2020

Keywords

  • Galaxies: high-redshift
  • Galaxies: kinematics
  • Galaxies: structure

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Structure and dynamics of high-z galaxies'. Together they form a unique fingerprint.

Cite this