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The role of radiation and halo mergers in Pop III star formation
Lilia Correa Magnus
, Britton D Smith
, Sadegh Khochfar
, Brian W O’Shea
, John H Wise
, Michael L Norman
,
Matthew J Turk
School of Information Sciences
Astronomy
National Center for Supercomputing Applications (NCSA)
Informatics
Social & Behavioral Science Institute
Research output
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Contribution to journal
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Article
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peer-review
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Keyphrases
Halo
100%
Star Formation
100%
Pop III Stars
100%
Gasses
50%
Star-forming
33%
Ultra-high Resolution
16%
Turbulence
16%
Molecular Hydrogen
16%
Hydrostatic Pressure
16%
Formation Pathway
16%
Ejecta
16%
Supernovae
16%
Molecular Gas
16%
Population III Stars
16%
Central Density
16%
Gas Content
16%
Two-stars
16%
Nearby Stars
16%
Cosmic Dawn
16%
Density Pressure
16%
Gas-rich
16%
Rise in Temperature
16%
Physics
Star Formation
100%
Population III Stars
66%
High Resolution
33%
Supernovae
33%
Ejecta
33%
Molecular Gas
33%
Fluid Statics
33%
Hydrogen
33%