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Collective outflow from a small multiple stellar system

Peters, Thomas; Klaassen, Pamela D; Mordecai-Mark, Mac Low; Schron, Martin; Federrath, Christoph; Smith, Michael D; Klessen, R.

Description

The formation of high-mass stars is usually accompanied by powerful protostellar outflows. Such high-mass outflows are not simply scaled-up versions of their lower-mass counterparts, since observations suggest that the collimation degree degrades with stellar mass. Theoretically, the origins of massive outflows remain open to question because radiative feedback and fragmentation of the accretion flow around the most massive stars, with M > 15 M , may impede the driving of magnetic disk winds....[Show more]

CollectionsANU Research Publications
Date published: 2014
Type: Journal article
URI: http://hdl.handle.net/1885/152204
Source: The Astrophysical Journal
DOI: 10.1088/0004-637X/788/1/14
Access Rights: Open Access

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