Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

On the interplay between star formation and feedback in galaxy formation simulations

Journal Article · · Astrophysical Journal
 [1]
  1. Department of Physics, University of Surrey, Guildford, GU2 7XH (United Kingdom)
We investigate the star formation–feedback cycle in cosmological galaxy formation simulations, focusing on the progenitors of Milky Way (MW)-sized galaxies. We find that in order to reproduce key properties of the MW progenitors, such as semi-empirically derived star formation histories (SFHs) and the shape of rotation curves, our implementation of star formation and stellar feedback requires (1) a combination of local early momentum feedback via radiation pressure and stellar winds, and subsequent efficient supernovae feedback, and (2) an efficacy of feedback that results in the self-regulation of the global star formation rate on kiloparsec scales. We show that such feedback-driven self-regulation is achieved globally for a local star formation efficiency per free fall time of ϵ{sub ff}≈10%. Although this value is larger that the ϵ{sub ff}∼1% value usually inferred from the Kennicutt–Schmidt (KS) relation, we show that it is consistent with direct observational estimates of ϵ{sub ff} in molecular clouds. Moreover, we show that simulations with local efficiency of ϵ{sub ff}≈10% reproduce the global observed KS relation. Such simulations also reproduce the cosmic SFH of the MW-sized galaxies and satisfy a number of other observational constraints. Conversely, we find that simulations that a priori assume an inefficient mode of star formation, instead of achieving it via stellar feedback regulation, fail to produce sufficiently vigorous outflows and do not reproduce observations. This illustrates the importance of understanding the complex interplay between star formation and feedback, and the detailed processes that contribute to the feedback-regulated formation of galaxies.
OSTI ID:
22883260
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 804; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United Kingdom
Language:
English

Similar Records

EXTENDED SCHMIDT LAW: ROLE OF EXISTING STARS IN CURRENT STAR FORMATION
Journal Article · Wed Jun 01 00:00:00 EDT 2011 · Astrophysical Journal · OSTI ID:21576753

The Physical Origin of Long Gas Depletion Times in Galaxies
Journal Article · Thu Aug 17 20:00:00 EDT 2017 · The Astrophysical Journal (Online) · OSTI ID:1354866

Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation–Feedback Cycle in Galaxies
Journal Article · Sun Aug 29 20:00:00 EDT 2021 · The Astrophysical Journal · OSTI ID:1826742