Panchromatic Tully-Fisher Relations

Details Panchromatic Tully-Fisher Relations Panchromatic Tully-Fisher Relations

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.0402m&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #04.02; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We present panchromatic Tully-Fisher relations from the Spitzer Infrared Nearby Galaxies Survey (SINGS) and its ancillary data archive. These data span a wide range of optical and infrared wavelengths including B, V, R, I, J, H, K, 3.6 and 4.5 microns. We explore trends in the slope and scatter of the observed relations, and discuss the implications of these on the properties of rotationally supported galaxies. Importantly, we extend the study of the Tully-Fisher relation to the 3.6 and 4.5 micron Spitzer wavebands, placing novel constraints on the stellar populations and dust content of these galaxies.

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