The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow f...
The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
We perform a series of three-dimensional, magnetohydrodynamical (MHD) simulations of star cluster formation including gravity, turbulence, magnetic fields, stellar radiative heating and outflow feedback. We observe that the inclusion of protostellar outflows (1) reduces the star formation rate by a factor of \(\sim2\), (2) increases fragmentation,...
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Full title
The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback
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TN_cdi_proquest_journals_2540620408
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2540620408
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2106.06521
