Fig. 3 from Mass Models for Low Surface Brightness Galaxies with High‐Resolution Optical Velocity Fields

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Mass Models for Low Surface Brightness Galaxies with High‐Resolution Optical Velocity Fields

Authors: Rachel Kuzio de Naray, Stacy S. McGaugh, and W. J. G. de Blok

Kuzio de Naray, McGaugh, & de Blok 2008 The Astrophysical Journal 676 920.

Provider: AAS Journals

Caption: Fig. 3.

Results for UGC 191, UGC 1551, and NGC 959. Top row: Position of DensePak array on the Hα images of the galaxies. Middle row: Observed DensePak velocity field. Empty fibers are those without detections. Bottom row: DensePak rotation curves. The open symbols in the UGC 191 and UGC 1551 rotation curves were excluded from the halo fits.

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