Abstract
We present the results of a 69 arcmin2 ALMA survey at 1.1 mm, GOODS-ALMA, matching the deepest HST-WFC3 H-band observed region of the GOODS-South field. The 35 galaxies detected by ALMA are among the most massive galaxies at z = 2–4 and are either starburst or located in the upper part of the galaxy star-forming main sequence. The analysis of the gas fraction, depletion time, X-ray luminosity and the size suggests that they are building compact bulges and are the ideal progenitors of compact passive galaxies at z˜2, and a slow downfall scenario is favoured in their future transition from star-forming to passive galaxies.
| Original language | English |
|---|---|
| Pages (from-to) | 67-71 |
| Number of pages | 5 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 15 |
| Early online date | 29 Mar 2021 |
| DOIs | |
| Publication status | Published - 2021 |
Keywords
- galaxies: ISM
- galaxies: evolution
- galaxies: high-redshift
- galaxies: nuclei
- submillimeter
Fingerprint
Dive into the research topics of 'GOODS-ALMA: AGNs and the slow downfall of massive star-forming galaxies at z > 2'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver