Idealized simulations with live gas particles show the LMC corona's present-day velocity and column density profiles match a first-passage orbit but are too low in a second-passage orbit, yielding truncation radii of 16.6 kpc versus 5.7 kpc and strongly disfavoring the latter.
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3 Pith papers cite this work, alongside 162 external citations. Polarity classification is still indexing.
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astro-ph.GA 3representative citing papers
Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.
Review chapter on HI observations of gas inflow/outflow in disk and dwarf galaxies and prospects for SKA-Mid AA4 to address missing data on low-column-density gas.
citing papers explorer
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The LMC Corona Favors a First Passage
Idealized simulations with live gas particles show the LMC corona's present-day velocity and column density profiles match a first-passage orbit but are too low in a second-passage orbit, yielding truncation radii of 16.6 kpc versus 5.7 kpc and strongly disfavoring the latter.
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Modeling the Accretion of High-Velocity Clouds from a Rotating Halo
Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.
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Deep HI observations of cold gas inflow and outflow
Review chapter on HI observations of gas inflow/outflow in disk and dwarf galaxies and prospects for SKA-Mid AA4 to address missing data on low-column-density gas.