We present a grid of radiation transfer models of axisymmetric young stellar objects (YSOs),
covering a wide range of stellar masses (from 0.1 to 50 M☉) and evolutionary stages (from …

A review of star formation in the Rho Ophiuchi molecular complex is presented, with
particular emphasis on studies of the main cloud, L1688, since 1991. Recent photometric …

We investigate protostellar outflow evolution, gas entrainment, and star formation efficiency
using radiation-hydrodynamic simulations of isolated, turbulent low-mass cores. We adopt …

We study protostellar envelope and outflow evolution using Hubble Space Telescope
NICMOS or WFC3 images of 304 protostars in the Orion molecular clouds. These near-IR …

We observed the Class I protostellar source Elias 29 with the Atacama Large Millimeter/
submillimeter Array. We detected CS, SO, 34 SO, SO 2, and SiO line emissions in a compact …

We present a catalogue of Molecular Hydrogen emission-line Objects (MHOs) in outflows
from young stars, most of which are deeply embedded. All objects are identified in the near …

Abstract We model Spitzer Space Telescope observations of the Taurus Class 0 protostar
L1527 IRS (IRAS 04368+ 2557) to provide constraints on its protostellar envelope structure …

Radio observations of low-mass star formation in molecular spectral lines have rapidly
progressed since the advent of the Atacama Large Millimeter/submillimeter Array (ALMA) …

Abstract CO, 13CO, and C18O J= 3–2 observations are presented of the Ophiuchus
molecular cloud. The 13CO and C18O emission is dominated by the Oph A clump, and the …

We present a two-epoch Hubble Space Telescope study of NGC 2071 IR highlighting HOPS
361-C, a protostar producing an arced 0.2 parsec-scale jet. The proper motions for the …