Ouflows, Infall & Disks in the G333 Cloud

Details Ouflows, Infall & Disks in the G333 Cloud Ouflows, Infall & Disks in the G333 Cloud

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1562b&link_type=abstract

ATNF proposal C1808, Semester: April, 2008

Computer Science

Stellar, Galactic, Atca

Scientific paper

In this proposal we seek to determine the viability of outflows from high-mass star-forming regions as a source of turbulence that can influence a subsequent generation of localised star formation. In doing this we will also investigate the powering of the outflows themselves, the nature of which is currently unknown. We will also obtain a comprehensive picture of the three key kinematic features of a forming massive stellar system, namely outflows, infall and rotating disks, the collective presence of which has rarely been detected in a single system but which is crucial to determining which of the two currently-favoured models (accretion vs coalescence) can successfully describe massive star formation. The proposed observations will augment data from an existing programme (proposal IDs C1580, C1583) to investigate outflows, infall and disks in massive star formation. This programme lies within the context of a larger international effort to quantify the role played by turbulence across all scales of star formation.

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