AAS 207th Meeting, 8-12 January 2006
Session 64 ISM outside the Milky Way
Poster, Tuesday, 9:20am-6:30pm, January 10, 2006, Exhibit Hall

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[64.09] THINGS: The HI Nearby Galaxy Survey

F. Walter (MPIA), E. Brinks (Univ. Hertfordshire), E. de Blok (Mt. Stromlo Obs.), F. Bigiel (MPIA), M. Thornley (Bucknell Univ.), R.C. Kennicutt (Cambridge)

We present first HI maps of the galaxies observed as part of The HI Nearby Galaxy Survey (THINGS). THINGS is a large program at the VLA to perform 21--cm HI observations of the highest quality (~7'', <5 km s-1 resolution) of nearby galaxies. The goal of THINGS is to investigate key characteristics related to galaxy morphology, star formation and mass distribution across the Hubble sequence. A sample of 34 objects with distances between 3 and 10 Mpc have been observed, covering a wide range of evolutionary stages and properties. THINGS is designed to complement SINGS, the Spitzer Infrared Nearby Galaxies Survey. For the THINGS sample, high--quality observations at comparable resolution will thus be available from the X--ray regime through to the radio part of the spectrum. THINGS data can be used to investigate issues such as the small--scale structure of the ISM, its three--dimensional structure, the (dark) matter distribution and processes leading to star formation. We present an HI composite of all THINGS galaxies which displays a stunning variety of structure in their interstellar medium.

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