Figure 6 from Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas

Authors: T. H. Jarrett, F. Masci, C. W. Tsai, S. Petty, M. E. Cluver, Roberto J. Assef, D. Benford, A. Blain, C. Bridge, E. Donoso, P. Eisenhardt, B. Koribalski, S. Lake, James D. Neill, M. Seibert, K. Sheth, A. Stanford, and N. Wright

Jarrett et al. 2013 The Astronomical Journal 145 6.

Provider: AAS Journals

Caption: Figure 6.

Central concentration index for the galaxy sample, corresponding to the ratio of the 3/4 light-radius to the 1/4 light-radius. For comparison, also shown is the bulge-to-disk ratio based on the double-Sérsic fit to the azimuthally averaged elliptical–radial profile (see Appendix C). The galaxy name is indicated below the measurement, where single numbers represent the NGC #. The Hubble T-Type is derived from the morphology (Table 1).

Other Images in This Article

Copyright and Terms & Conditions