The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS (2021)

First Author: Katsianis A

Attributed to: DiRAC-3 Operations 2019-2022 - Edinburgh funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa3236

Publication URI: http://dx.doi.org/10.1093/mnras/staa3236

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2