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Evolution of giant molecular clouds across cosmic time

Guszejnov, Dávid and Grudić, Michael Y. and Offner, Stella S. R. and Boylan-Kolchin, Michael and Faucher-Giguère, Claude-André and Wetzel, Andrew and Benincasa, Samantha M. and Loebman, Sarah (2020) Evolution of giant molecular clouds across cosmic time. Monthly Notices of the Royal Astronomical Society, 492 (1). pp. 488-502. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200227-131351859

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Abstract

Giant molecular clouds (GMCs) are well studied in the local Universe, however, exactly how their properties vary during galaxy evolution is poorly understood due to challenging resolution requirements, both observational and computational. We present the first time-dependent analysis of GMCs in a Milky Way-like galaxy and an Large Magellanic Cloud (LMC)-like dwarf galaxy of the FIRE-2 (Feedback In Realistic Environments) simulation suite, which have sufficient resolution to predict the bulk properties of GMCs in cosmological galaxy formation self-consistently. We show explicitly that the majority of star formation outside the galactic centre occurs within self-gravitating gas structures that have properties consistent with observed bound GMCs. We find that the typical cloud bulk properties such as mass and surface density do not vary more than a factor of 2 in any systematic way after the first Gyr of cosmic evolution within a given galaxy from its progenitor. While the median properties are constant, the tails of the distributions can briefly undergo drastic changes, which can produce very massive and dense self-gravitating gas clouds. Once the galaxy forms, we identify only two systematic trends in bulk properties over cosmic time: a steady increase in metallicity produced by previous stellar populations and a weak decrease in bulk cloud temperatures. With the exception of metallicity, we find no significant differences in cloud properties between the Milky Way-like and dwarf galaxies. These results have important implications for cosmological star and star cluster formation and put especially strong constraints on theories relating the stellar initial mass function to cloud properties.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stz3527DOIArticle
https://arxiv.org/abs/1910.01163arXivDiscussion Paper
ORCID:
AuthorORCID
Guszejnov, Dávid0000-0001-5541-3150
Grudić, Michael Y.0000-0002-1655-5604
Offner, Stella S. R.0000-0003-1252-9916
Boylan-Kolchin, Michael0000-0002-9604-343X
Faucher-Giguère, Claude-André0000-0002-4900-6628
Wetzel, Andrew0000-0003-0603-8942
Benincasa, Samantha M.0000-0003-4826-9079
Loebman, Sarah0000-0003-3217-5967
Additional Information:© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2019 December 10. Received 2019 December 6; in original form 2019 October 3. Published: 17 December 2019. The authors would like to thank Philip F. Hopkins for his helpful comments. This work used computational resources of the University of Texas at Austin and the Texas Advanced Computing Center (TACC; http://www.tacc.utexas.edu). DG is supported by the Harlan J. Smith McDonald Observatory Postdoctoral Fellowship. MYG is supported by a CIERA Postoctoral Fellowship. SSRO is supported by NSF Career Award AST-1650486 and by a Cottrell Scholar Award from the Research Corporation for Science Advancement. MBK acknowledges support from NSF grant no. AST-1517226 and CAREER grant no. AST-1752913 and from NASA grant nos NNX17AG29G and HST-AR-14282, HST-AR-14554, HST-AR-15006, and HST-GO-14191 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS5-26555. CAFG was supported by NSF through grant nos AST-1517491, AST-1715216, and CAREER award AST-1652522, by NASA through grant nos NNX15AB22G and 17-ATP17-0067, and by a Cottrell Scholar Award from the Research Corporation for Science Advancement. AW received support from NASA, through ATP grant no. 80NSSC18K1097 and HST grant nos GO-14734 and AR-15057 from STScI, a Hellman Fellowship from UC Davis, and the Heising-Simons Foundation. Support for SRL was provided by NASA through Hubble Fellowship grant no. HST-JF2-51395.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555.
Group:TAPIR
Funders:
Funding AgencyGrant Number
University of Texas at AustinUNSPECIFIED
Northwestern UniversityUNSPECIFIED
NSFAST-1650486
Cottrell Scholar of Research CorporationUNSPECIFIED
NSFAST-1517226
NSFAST-1752913
NASANNX17AG29G
NASAHST-AR-14282
NASAHST-AR-14554
NASAHST-AR-15006
NASAHST-GO-14191
NASANAS5-26555
NSFAST-1517491
NSFAST-1715216
NSFAST-1652522
NASANNX15AB22G
NASA17-ATP17-0067
NASA80NSSC18K1097
NASA Hubble FellowshipGO-14734
NASA Hubble FellowshipAR-15057
University of California, DavisUNSPECIFIED
Heising-Simons FoundationUNSPECIFIED
NASA Hubble FellowshipHST-JF2-51395.001-A
Subject Keywords:turbulence – stars: formation – ISM: clouds – galaxies: ISM– galaxies: star formation – cosmology: theory
Issue or Number:1
Record Number:CaltechAUTHORS:20200227-131351859
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200227-131351859
Official Citation:Dávid Guszejnov, Michael Y Grudić, Stella S R Offner, Michael Boylan-Kolchin, Claude-André Faucher-Gigère, Andrew Wetzel, Samantha M Benincasa, Sarah Loebman, Evolution of giant molecular clouds across cosmic time, Monthly Notices of the Royal Astronomical Society, Volume 492, Issue 1, February 2020, Pages 488–502, https://doi.org/10.1093/mnras/stz3527
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:101621
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:27 Feb 2020 21:51
Last Modified:27 Feb 2020 21:51

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