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Papers
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Can Cosmological Simulations Reproduce the Spectroscopically Confirmed
Galaxies Seen at z≥ 10?
arXiv
ApJ
ADS
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Is There a Missing Outskirts Problem? Stellar Haloes as
a Sensitive Probe of Supernova Feedback
arXiv
ADS
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Uncertainties in SN rates drive qualitative
differences in simulations of galaxy evolution
arXiv
ADS
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Where did the globular clusters of the Milky Way form?
arXiv
mnras
ADS
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Entropy-driven winds: Outflows and fountains lifted gently by buoyancy
arXiv
mnras
ADS
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Chaos and Variance in Galaxy Formation
arXiv
mnras
ADS
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ΛCDM is consistent with SPARC Acceleration Law
arXiv
ApJL
ADS
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Cosmological Galaxy Evolution With Superbubble Feedback II
arXiv
mnras
ADS
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Cosmological Galaxy Evolution With Superbubble Feedback I
arXiv
mnras
ADS
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A Superbubble Feedback Model for Galaxy Simulations
arXiv
mnras
ADS
Slide Decks
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Accretion, Buoyancy, and Chaos: ABCs of Galaxy Formation @ Santa Cruz Galaxy Workshop 2015
PDF
ODP
VID
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Superbubble Regulation of Baryons in Cosmological Galaxy Formation
@ Computing the Universe 2016
PDF
ODP
VID
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Superbubble Driven Galactic Winds: Realistic Galaxies from Moderate Feedback
Energy @ Santa Cruz Galaxy Workshop 2015
PDF
VID
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Cosmological Galaxy Evolution with Superbubble Feedback @ CASCA 2015
PDF
PPT
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Superbubble Feedback in Galaxy Formation @ CASCA 2014
PDF
PPT
Selected Videos