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Where do we go from here? • MORE! Galaxies to stars : formation + dispersion of of molecular cloud in galaxy environment - how does accretion/galactic environment shape star formation? • Simulations + non-ideal magnetic effects that resolve protostellar accretion disks - what fraction of multiples form via core vs. disk fragmentation? • Better treatment of microphysics ("astrochemistry"): how does habitability evolve with cosmic time?

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Where do we go from here? • MORE! Galaxies to stars : formation + dispersion of of molecular cloud in galaxy environment - how does accretion/galactic environment shape star formation? • Simulations + non-ideal magnetic effects that resolve protostellar accretion disks - what fraction of multiples form via core vs. disk fragmentation? • Better treatment of microphysics ("astrochemistry"): how does habitability evolve with cosmic time?
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Kelly Lepo (kellylepo@astrodon.social)'s status on Tuesday, 21-Jan-2025 01:35:07 JST Kelly Lepo
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Future work includes more work on galactic environments and trying to incorporate very tricky microphysics like astrochemistry into the simulations.

In conversation about 18 days ago from astrodon.social permalink