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Rapid disc settling and the transition from bursty to steady star formation in Milky Way-mass galaxies

Gurvich, Alexander B; Stern, Jonathan; Faucher-Giguère, Claude-André; Hopkins, Philip F; Wetzel, Andrew; Moreno, Jorge; Hayward, Christopher C; Richings, Alexander J; Hafen, Zachary

Rapid disc settling and the transition from bursty to steady star formation in Milky Way-mass galaxies Thumbnail


Authors

Alexander B Gurvich

Jonathan Stern

Claude-André Faucher-Giguère

Philip F Hopkins

Andrew Wetzel

Jorge Moreno

Christopher C Hayward

Alexander J Richings

Zachary Hafen



Abstract

Recent observations and simulations indicate substantial evolution in the properties of galaxies with time, wherein rotationally supported and steady thin discs (like those frequently observed in the local Universe) emerge from galaxies that are clumpy, irregular, and have bursty star formation rates (SFRs). To better understand the progenitors of local disc galaxies, we carry out an analysis of three FIRE-2 simulated galaxies with a mass similar to the Milky Way at redshift z = 0. We show that all three galaxies transition from bursty to steady SFRs at a redshift between z = 0.5 and z = 0.8, and that this transition coincides with the rapid (≲1 Gyr) emergence of a rotationally supported interstellar medium (ISM). In the late phase with steady SFR, the rotational energy comprises
of the total kinetic + thermal energy in the ISM, and is roughly half the gravitational energy. By contrast, during the early bursty phase, the ISM initially has a quasi-spheroidal morphology and its energetics are dominated by quasi-isotropic in- and outflows out of virial equilibrium. The subdominance of rotational support and out-of-equilibrium conditions at early times challenge the application of standard equilibrium disc models to high-redshift progenitors of Milky Way-like galaxies. We further find that the formation of a rotationally-supported ISM coincides with the onset of a thermal pressure supported inner circumgalactic medium (CGM). Before this transition, there is no clear boundary between the ISM and the inner CGM.

Citation

Gurvich, A. B., Stern, J., Faucher-Giguère, C., Hopkins, P. F., Wetzel, A., Moreno, J., …Hafen, Z. (2023). Rapid disc settling and the transition from bursty to steady star formation in Milky Way-mass galaxies. Monthly Notices of the Royal Astronomical Society, 519(2), 2598-2614. https://doi.org/10.1093/mnras/stac3712

Journal Article Type Article
Acceptance Date Dec 13, 2022
Online Publication Date Dec 23, 2022
Publication Date 2023-02
Deposit Date Jan 24, 2024
Publicly Available Date Jan 24, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 519
Issue 2
Pages 2598-2614
DOI https://doi.org/10.1093/mnras/stac3712
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL https://durham-repository.worktribe.com/output/2163245

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Copyright Statement
© 2022 The Author(s)
Published by Oxford University Press on behalf of Royal Astronomical Society





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