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Suppression of star formation in dwarf galaxies by photoelectric grain heating feedback

Author

Listed:
  • John C. Forbes

    (University of California)

  • Mark R. Krumholz

    (University of California
    Research School of Astronomy and Astrophysics, Australian National University)

  • Nathan J. Goldbaum

    (National Center for Supercomputing Applications, University of Illinois)

  • Avishai Dekel

    (Center for Astrophysics and Planetary Sciences, Racah Institute of Physics, The Hebrew University)

Abstract

Simulations of dwarf galaxies that include photoelectric grain heating and supernovae indicate that the former is the dominant means by which these galaxies regulate their star formation rate, because the latter are unable to account for the observed large gas depletion times.

Suggested Citation

  • John C. Forbes & Mark R. Krumholz & Nathan J. Goldbaum & Avishai Dekel, 2016. "Suppression of star formation in dwarf galaxies by photoelectric grain heating feedback," Nature, Nature, vol. 535(7613), pages 523-525, July.
    • Handle: RePEc:nat:nature:v:535:y:2016:i:7613:d:10.1038_nature18292
    DOI: 10.1038/nature18292
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    Cited by:

    1. Elena N. Akimova & Vladimir E. Misilov & Igor M. Kulikov & Igor G. Chernykh, 2022. "OMPEGAS: Optimized Relativistic Code for Multicore Architecture," Mathematics, MDPI, vol. 10(14), pages 1-12, July.

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