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High-Mass Star Formation
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A review on current theories and observations of high-mass star formation is given. Particularly the influence of magnetic fields and feedback mechanisms, and of varying initial conditions on theories are discussed. The, in my biased view, most important observations to put strong constraints on models of high-mass star formation are pres ented, in particular bearing on the existence and properties of high-mass starless cores, the role of filaments in the mass transport to high-mass cores, and the propertie s of disks around high-mass stars.
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Cited by 1 Pith paper
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Physical properties and gas kinematics of massive star forming region G328.24$-$0.55
ALMA data reveal five protostellar cores in G328.24 minus 0.55, with MM1a as a line-rich, hot, early-stage massive protostar that appears to drive a bipolar outflow and host a rotating envelope.
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