Physics
Scientific paper
Sep 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004msngr.117...36c&link_type=abstract
The Messenger (ISSN0722-6691), No.117, p. 36-39 (September 2004)
Physics
2
Scientific paper
New results from ESO and IRAM suggest that massive stars form in the same way as their low-mass counterparts. In the Omega nebula, a young stellar object of more than ten solar masses is surrounded by a huge rotating disc with at least 100 solar masses of gas and dust. Part of the gas that falls onto the growing star is ejected perpendicularly to the disc, producing a bipolar jet and an hourglass shaped nebula.
Chini Rolf
Hoffmeister Vera
Kimeswenger Stefan
Nielbock Markus
Nürnberger Dieter
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