Nature of high-mass dense cores in NGC6334/6357

Details Nature of high-mass dense cores in NGC6334/6357 Nature of high-mass dense cores in NGC6334/6357

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1583r&link_type=abstract

ATNF proposal M324, Semester: April, 2008

Computer Science

Galactic, Mopra

Scientific paper

We propose to investigate the nature of the most massive dense cores of the twin molecular complex NGC6334/6357. These cores are the present locations of high-mass star formation and, as such, will provide important insights on its earliest phases. Specifying the nature of the massive dense cores of NGC6334/6357 will allow us to check and extend the results recently obtained in Cygnus X by Motte et al. (2007). Indeed, they have shown that IR-quiet high-mass protostars driving intense SiO outflows do exist, and that pure pre-stellar high-mass cores are rare, thus being short-living objects probably created in a dynamical way.

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