CaltechAUTHORS
Published May 20, 2022 | Version Accepted Version + Published
Journal Article Open

Implications of a Temperature-dependent Initial Mass Function. II. An Updated View of the Star-forming Main Sequence

Creators

  • 1. ROR icon University of Copenhagen
  • 2. ROR icon California Institute of Technology
  • 3. ROR icon University of California, Riverside

Abstract

The stellar initial mass function (IMF) is predicted to depend upon the temperature of gas in star-forming molecular clouds. The introduction of an additional parameter, TIMF, into photometric template fitting, allows galaxies to be fit with a range of IMFs. Three surprising new features appear: (1) most star-forming galaxies are best fit with a bottom-lighter IMF than the Milky Way; (2) most star-forming galaxies at fixed redshift are fit with a very similar IMF; and (3) the most-massive star-forming galaxies at fixed redshift instead exhibit a less bottom-light IMF, similar to that measured in quiescent galaxies. Additionally, since stellar masses and star formation rates both depend on the IMF, these results slightly modify the resulting relationship, while yielding similar qualitative characteristics to previous studies.

Additional Information

© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received 2021 September 21; revised 2022 March 11; accepted 2022 March 28; published 2022 May 25. The authors would like to thank Vasily Kokorev and Darach Watson for useful discussions. C.L.S. is supported by ERC grant 648179 "ConTExt." B.M. is supported by the Tombrello Fellowship. A.L. is supported by the Selove Prize. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant No. 140. The Flatiron Institute is supported by the Simons Foundation.

Attached Files

Published - Steinhardt_2022_ApJ_931_58.pdf

Accepted Version - 2205.14161.pdf

Files

2205.14161.pdf

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Additional details

Additional titles

Alternative title
Implications of a Temperature Dependent IMF II: An Updated View of the Star-Forming Main Sequence

Identifiers

Eprint ID
115294
Resolver ID
CaltechAUTHORS:20220629-450215700

Related works

Describes
https://arxiv.org/abs/2205.14161 (URL)

Funding

European Research Council (ERC)
648179
Tombrello Fellowship
Selove Prize
Danish National Research Foundation
140
Simons Foundation

Dates

Created
2022-06-30
Created from EPrint's datestamp field
Updated
2022-06-30
Created from EPrint's last_modified field