Starburst Galaxies Under the Microscope: High-Resolution Observations with VISIR and SINFONI

Physics

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Scientific paper

Infrared observations of starburst galaxies not only enable penetration
of the obscuring veil of dust, but also provide unique diagnostics in
the form of nebular emission lines and emission from dust and polycyclic
aromatic hydrocarbons (PAHs). Here we describe some first results of our
ongoing study of starburst galaxies with VISIR and SINFONI at the VLT.

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