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Uncovering Spiral Structure in Flocculent Galaxies

  • Authors: Michele D. Thornley

Thornley 1996 The Astrophysical Journal Letters 469 L45.

  • Provider: AAS Journals

Caption: Fig. 2.

Plot of K﹩\arcmin﹩ radial surface brightness profiles for NGC 4414 and NGC 5055. The crosses indicate the measured radial profile, the dashed line indicates the model disk, and the dotted line indicates the model bulge. The solid line indicates the total model distribution.

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