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 | |
| Publication status | Published - 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
Access to Document
- Wuyts.pdf
This article has been published in Proceedings of the International Astronomical Union https://doi.org/10.1017/S1743921319009293. This version is free to view and download for private research and study only. Not for re-distribution, re-sale or use in derivative works. © International Astronomical Union 2020.