An Overview of The H I Nearby Galaxy Survey (THINGS)

Details An Overview of The H I Nearby Galaxy Survey (THINGS) An Overview of The H I Nearby Galaxy Survey (THINGS)

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..407...88d&link_type=abstract

The Low-Frequency Radio Universe ASP Conference Series, Vol. 407, proceedings of the conference held 8-12 December 2008, at Nati

Astronomy and Astrophysics

Astrophysics

Scientific paper

The HI Nearby Galaxy Survey (THINGS) is a high spectral (≤ 5.2 km s-1) and spatial (˜ 6'') resolution survey of HI emission in 34 nearby galaxies obtained using the NRAO Very Large Array (VLA). The overarching scientific goal of THINGS is to investigate fundamental characteristics of the interstellar medium (ISM) related to galaxy morphology, star formation and mass distribution across the Hubble sequence. Here we summarize some of the recent results obtained with THINGS.

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