We present λ 1.3 mm Combined Array for Research in Millimeter-wave Astronomy
observations of dust polarization toward 30 star-forming cores and eight star-forming regions …

We mapped the kinetic temperature structure of two massive star-forming regions, N113 and
N159W, in the Large Magellanic Cloud (LMC). We have used~ 1.′′ 6 (~ 0.4 pc) resolution …

Context. High-mass star formation typically takes place in a crowded environment, with a
higher likelihood of young forming stars affecting and being affected by their surroundings …

We mapped the kinetic temperature structure of the Orion molecular cloud 1 (OMC-1) with
para-H 2 CO (JK a K c= 3 03–2 02, 3 22–2 21, and 3 21–2 20) using the APEX 12 m …

Context. The kinetic temperature of molecular clouds is a fundamental physical parameter
affecting star formation and the initial mass function. The Large Magellanic Cloud (LMC) is …

Context. For a general understanding of the physics involved in the star formation process,
measurements of physical parameters such as temperature and density are indispensable …

We present high angular resolution Submillimeter Array and Karl G. Jansky Very Large
Array observations of the massive protocluster G18. 67+ 0.03. Previously targeted in maser …

We present in this paper the results of high spectral resolution (R= 88,100) spectroscopy at
4.7 μm with iSHELL/IRTF of hot molecular gas close to the massive binary protostar W3 IRS …

We present in this paper mid-infrared (5–8 μm) spectroscopy toward the massive young
binary W3 IRS 5, using the Echelon Cross Echelle Spectrograph (EXES) spectrometer in …

Context. Two competing models describe the formation of massive stars in objects like the
Orion Trapezium. In the turbulent core accretion model, the resulting stellar masses are …