Rotating disks in high-mass young stellar objects

(2) IRAM; (3) Istituto di Radioastronomia; 4); (4) Caltech; Claudio Codella (3); Firenze; France; Grenoble; Italy; Leonardo Testi (1)

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Rotating disks in high-mass young stellar objects

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arxiv astro-ph/0312495 v1 submitted 2003-12-18 astro-ph

Maria T. Beltran (1) , Riccardo Cesaroni (1) , Roberto Neri (2) , Claudio Codella (3) , Ray S. Furuya (1 , 4) , Leonardo Testi (1) , Luca Olmi (3) ((1) Osservatorio Astrofisico di Arcetri

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Firenze Italy (2) IRAM Grenoble France (3) Istituto di Radioastronomia (4) Caltech Pasadena USA)

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keywords diskshigh-massrotatingaccretionbipolardetectionembeddedformation

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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 ~10E-2 Msun/yr.

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