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Converting sink particles to stars in hydrodynamical simulations

Published online by Cambridge University Press:  20 January 2023

Kong You Liow Open the ORCID record for Kong You Liow [Opens in a new window] ,
Steven Rieder Open the ORCID record for Steven Rieder [Opens in a new window] ,
Clare Dobbs  and
Sarah Jaffa
Kong You Liow
Affiliation:
University of Exeter, Exeter EX4 4QL, UK
Steven Rieder
Affiliation:
University of Exeter, Exeter EX4 4QL, UK RIKEN Center for Computational Science, 650-0047, Hyogo, Japan
Clare Dobbs
Affiliation:
University of Exeter, Exeter EX4 4QL, UK
Sarah Jaffa
Affiliation:
University of Hertfordshire, Hertfordshire AL10 9AA, UK University College London, London WC1H 9NE, UK
Rights & Permissions [Opens in a new window]

Abstract

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To form stars in hydrodynamical simulations, we introduce the grouped star formation prescription to convert the grouped sink particles into stars that follow the IMF. We show that this method is robust in different physical scales. Such methods to form stars are likely to become more important as galactic or even cosmological scale simulations begin to probe sub-parsec scales.

Keywords

galaxies: ISMISM: cloudsstars: formationgalaxies: star clusters: general
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S362: The Predictive Power of Computational Astrophysics as a Discovery Tool , June 2020 , pp. 380 - 381
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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