Star Formation
Fundamentals of Astrophysics(2021)
Abstract
SFR = ff Mselection tff • Galactic Disk kpc simulation (TIGRESS) • Density selection: thresholds, bins • Gravity/Energy selection: Φ isocontours bind gas • Compare various models for “predicting” SFR • Simple density competitive with other models • Model parameters vary with threshold density ( ff ∼ 0.03 − 0.4) Identifying Gas Structures Correlated with SFR in ISM disk simulations Alwin Mao, Eve Ostriker, and Chang-Goo Kim Princeton University
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