Disk-halo interactions in the starburst galaxy NGC 6810

Details Disk-halo interactions in the starburst galaxy NGC 6810 Disk-halo interactions in the starburst galaxy NGC 6810

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop..651d&link_type=abstract

ATNF proposal C1643, Semester: April, 2007

Physics

Extragalactic, Atca

Scientific paper

NGC 6810, a highly inclined southern starburst galaxy, exhibits extraplanar soft X-ray and Halpha emission. For a multi-wavelength study of the halo and its dependence on the star formation properties of the underlying disk high-resolution radio data are required due to the small source extent (150"x30"). We propose to fill the gap in the uv-plane of archival 375+750+1.5 km array ATCA data reduced by us with one full synthesis in a 6-km configuration for a detailed study in both HI and radio continuum.

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