Journal
ASTROPHYSICAL JOURNAL
Volume 601, Issue 2, Pages L187-L190Publisher
IOP PUBLISHING LTD
DOI: 10.1086/382150
Keywords
ISM : individual (G24.78+0.08, G31.41+0.31); ISM : molecules; radio lines : ISM; stars : formation
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We report on the detection of four rotating massive disks in two regions of high-mass star formation. The disks are perpendicular to known bipolar outflows and turn out to be unstable but long-lived. We infer that accretion onto the embedded (proto) stars must proceed through the disks with rates of similar to10(-2) M-. yr(-1).
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