Looking into the dust - revealing the inner structure and kinematics of ATLASGAL clumps

Details Looking into the dust - revealing the inner structure and kinematics of ATLASGAL clumps Looking into the dust - revealing the inner structure and kinematics of ATLASGAL clumps

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3293t&link_type=abstract

ATNF proposal C2370, Semester: April, 2010

Physics

Star Formation, Atca

Scientific paper

The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) revealed thousands of new dust continuum sources, that most likely are places of high-mass star/cluster formation. For the first time an unbiased statistical sample is available that can be used to study the earliest phases of star formation. From this sample, carefully selected sources in potential early evolutionary stages are proposed for ATCA follow up observation to identify cores in the submm clumps, investigate if there is a correlation between FIR defined classes and the degree of fragmentation and tighten the constrains on FIR/submm SEDs. Line observations of HCN(1-0) and N_2H^+(1-0) provide density tracers and information about the kinematic of the cores.

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