Stellar feedback is needed to produce realistic giant molecular clouds and galaxies in
simulations, but due to limited numerical resolution, feedback must be implemented using …

We present∼ 10–40 μm SOFIA-FORCAST images of 11 isolated protostars as part of the
SOFIA Massive (SOMA) Star Formation Survey, with this morphological classification based …

We present a detailed study of the massive star-forming region G35. 2-0.74 N with Atacama
Large Millimeter/submillimeter Array (ALMA) 1.3 mm multi-configuration observations. At 0 …

We report results of 0. 05-resolution observations toward the O-type proto-binary system
IRAS 16547–4247 with the Atacama Large Millimeter/submillimeter Array. We present …

We present multiwavelength images observed with SOFIA-FORCAST from∼ 10 to 40 μm of
seven high luminosity massive protostars, as part of the SOFIA Massive Star Formation …

Abstract We present–m~ 10 40 m SOFIA–FORCAST images of 14 intermediate-mass
protostar candidates as part of the SOFIA Massive (SOMA) Star Formation Survey. We build …

To study the early phases of massive star formation, we present ALMA observations of SiO
(5− 4) emission and VLA observations of 6 cm continuum emission toward 32 Infrared Dark …

Massive young stellar objects (MYSOs) are known to undergo an evolutionary phase in
which high mass accretion rates drive strong outflows. A class of objects believed to trace …

We present results from a sample of 106 high-luminosity IRAS sources observed with the
Very Large Array in the B and C configurations. 96 sources were observed in the X-band …

Massive protostars generate strong radiation feedback, which may help set the mass that
they achieve by the end of the accretion process. Studying such feedback is therefore crucial …