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edge: the emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations

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Τίτλος: edge: the emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
Συγγραφείς: Rey, Martin P., Taylor, Ethan, Gray, Emily I., Kim, Stacy Y., Andersson, Eric P., Pontzen, Andrew, Agertz, Oscar, Read, Justin I., Cadiou, Corentin, Yates, Robert M., Orkney, Matthew D.A., Scholte, Dirk, Saintonge, Amélie, Breneman, Joseph, Mcquinn, Kristen B.W., Muni, Claudia, Das, Payel
Συνεισφορές: Lund University, Faculty of Science, Department of Physics, Astrophysics, Lunds universitet, Naturvetenskapliga fakulteten, Fysiska institutionen, Astrofysik, Originator, Lund University, Faculty of Science, Department of Physics, Lunds universitet, Naturvetenskapliga fakulteten, Fysiska institutionen, Originator
Πηγή: Monthly Notices of the Royal Astronomical Society. 541(2):1195-1217
Θεματικοί όροι: Natural Sciences, Physical Sciences, Astronomy, Astrophysics and Cosmology, Naturvetenskap, Fysik, Astronomi, astrofysik och kosmologi
Περιγραφή: We present a new suite of edge ('Engineering Dwarfs at Galaxy formation's Edge') cosmological zoom simulations. The suite includes 15 radiation-hydrodynamical dwarf galaxies covering the ultrafaint to the dwarf irregular regime () to enable comparisons with observed scaling relations. Each object in the suite is evolved at high resolution () and includes stellar radiation, winds, and supernova feedback channels. We compare with previous edge simulations without radiation, finding that radiative feedback results in significantly weaker galactic outflows. This generalizes our previous findings to a wide mass range, and reveals that the effect is most significant at low. Despite this difference, stellar masses stay within a factor of two of each other, and key scaling relations of dwarf galaxies (size-mass, neutral gas-stellar mass, and gas-phase mass-metallicity) emerge correctly in both simulation suites. Only the stellar mass-stellar metallicity relation is strongly sensitive to the change in feedback. This highlights how obtaining statistical samples of dwarf galaxy stellar abundances with next-generation spectrographs will be key to probing and constraining the baryon cycle of dwarf galaxies.
Σύνδεσμος πρόσβασης: https://doi.org/10.1093/mnras/staf1058
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  Data: edge: the emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
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  Data: Lund University, Faculty of Science, Department of Physics, Astrophysics, Lunds universitet, Naturvetenskapliga fakulteten, Fysiska institutionen, Astrofysik, Originator<br />Lund University, Faculty of Science, Department of Physics, Lunds universitet, Naturvetenskapliga fakulteten, Fysiska institutionen, Originator
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  Data: <i>Monthly Notices of the Royal Astronomical Society</i>. 541(2):1195-1217
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  Data: We present a new suite of edge ('Engineering Dwarfs at Galaxy formation's Edge') cosmological zoom simulations. The suite includes 15 radiation-hydrodynamical dwarf galaxies covering the ultrafaint to the dwarf irregular regime () to enable comparisons with observed scaling relations. Each object in the suite is evolved at high resolution () and includes stellar radiation, winds, and supernova feedback channels. We compare with previous edge simulations without radiation, finding that radiative feedback results in significantly weaker galactic outflows. This generalizes our previous findings to a wide mass range, and reveals that the effect is most significant at low. Despite this difference, stellar masses stay within a factor of two of each other, and key scaling relations of dwarf galaxies (size-mass, neutral gas-stellar mass, and gas-phase mass-metallicity) emerge correctly in both simulation suites. Only the stellar mass-stellar metallicity relation is strongly sensitive to the change in feedback. This highlights how obtaining statistical samples of dwarf galaxy stellar abundances with next-generation spectrographs will be key to probing and constraining the baryon cycle of dwarf galaxies.
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