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Most Stars (and Planets?) Are Born in Intense Radiation Fields
Eve J. Lee, Philip F. Hopkins
Protostars and young stars are strongly spatially "clustered" or "correlated" within their natal giant molecular clouds (GMCs). We demonstrate that such clustering leads to the con…
Time Varying Dynamical Star Formation Rate
Eve J. Lee, Philip Chang, Norman Murray
We present numerical evidence of dynamic star formation in which the accreted stellar mass grows superlinearly with time, roughly as . We perform simulations of star formation…
Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons
S. S. R. Offner, E. J. Lee, A. A. Goodman +1
We present results from three-dimensional, self-gravitating, radiation-hydrodynamic simulations of low-mass protostellar outflows. We construct synthetic observations in 12CO in or…
Substellar Objects in Nearby Young Clusters (SONYC) II: The Brown Dwarf Population of Rho Ophiuchi
Vincent Geers, Alexander Scholz, Ray Jayawardhana +3
SONYC - Substellar Objects in Nearby Young Clusters - is a survey program to investigate the frequency and properties of brown dwarfs down to masses below the Deuterium burning lim…