Abstract
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 ~10-2 Msolar yr-1. Based on observations carried out with the IRAM Plateau de Bure Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain).
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CITATION STYLE
Beltrn, M. T., Cesaroni, R., Neri, R., Codella, C., Furuya, R. S., Testi, L., & Olmi, L. (2004). Rotating Disks in High-Mass Young Stellar Objects. The Astrophysical Journal, 601(2), L187–L190. https://doi.org/10.1086/382150
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