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The elephant in the room: the importance of the details of massive star formation in molecular clouds

Grudić, Michael Y. and Hopkins, Philip F. (2019) The elephant in the room: the importance of the details of massive star formation in molecular clouds. Monthly Notices of the Royal Astronomical Society, 488 (2). pp. 2970-2975. ISSN 0035-8711. doi:10.1093/mnras/stz1820.

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Most simulations of galaxies and massive giant molecular clouds (GMCs) cannot explicitly resolve the formation (or predict the main-sequence masses) of individual stars. So they must use some prescription for the amount of feedback from an assumed population of massive stars (e.g. sampling the initial mass function, IMF). We perform a methods study of simulations of a star-forming GMC with stellar feedback from UV radiation, varying only the prescription for determining the luminosity of each stellar mass element formed (according to different IMF sampling schemes). We show that different prescriptions can lead to widely varying (factor of ∼3) star formation efficiencies (on GMC scales) even though the average mass-to-light ratios agree. Discreteness of sources is important: radiative feedback from fewer, more-luminous sources has a greater effect for a given total luminosity. These differences can dominate over other, more widely recognized differences between similar literature GMC-scale studies (e.g. numerical methods, cloud initial conditions, presence of magnetic fields). Moreover the differences in these methods are not purely numerical: some make different implicit assumptions about the nature of massive star formation, and this remains deeply uncertain in star formation theory.

Item Type:Article
Related URLs:
URLURL TypeDescription
Grudić, Michael Y.0000-0002-1655-5604
Hopkins, Philip F.0000-0003-3729-1684
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 ( Accepted 2019 July 1. Received 2019 June 5; in original form 2018 September 21. Published: 25 July 2019. We thank Mark Krumholz, Stella Offner, Claude-André Faucher-Giguère, Norman Murray, Eliot Quataert, James Dale, Ian Bonnell, Hui Li, Jeong-Gyu Kim, Eve Ostriker, Michael S. Fall, Christopher Matzner, Benny Tsang, and Milos Milosavljević for enlightening discussions that informed and motivated this work. Support for MYG and PFH was provided by a James A Cullen Memorial Fellowship, an Alfred P. Sloan Research Fellowship, NSF Collaborative Research Grant #1715847 and CAREER grant #1455342, and NASA grants NNX15AT06G, JPL 1589742, 17-ATP17-0214. Numerical calculations were run on the Caltech compute cluster ‘Wheeler,’ allocations from XSEDE TG-AST130039 and PRAC NSF.1713353 supported by the NSF, and NASA HEC SMD-16-7592. This research has made use of the NASA Astrophysics Data System, IPYTHON (Pérez & Granger 2007), NUMPY, SCIPY (Jones et al. 2001), NUMBA (Lam, Pitrou & Seibert 2015), and MATPLOTLIB (Hunter 2007).
Group:TAPIR, Astronomy Department
Funding AgencyGrant Number
James A. Cullen Memorial FellowshipUNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
Subject Keywords:stars: formation, stars: massive, ISM: clouds, galaxies: formation
Issue or Number:2
Record Number:CaltechAUTHORS:20190911-150204286
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Official Citation:Michael Y Grudić, Philip F Hopkins, The elephant in the room: the importance of the details of massive star formation in molecular clouds, Monthly Notices of the Royal Astronomical Society, Volume 488, Issue 2, September 2019, Pages 2970–2975,
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:98585
Deposited By: Tony Diaz
Deposited On:11 Sep 2019 23:13
Last Modified:16 Nov 2021 17:40

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