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Accurate Determination of the Mass Distribution in Spiral Galaxies. II. Testing the Shape of Dark Halos

  • Authors: Sébastien Blais-Ouellette, Philippe Amram, and Claude Carignan

Blais‐Ouellette, Amram, & Carignan 2001 The Astronomical Journal 121 1952.

  • Provider: AAS Journals

Caption: Fig. 10.

Best‐fit mass models using MOND and two different values of a0: a0 = 1.2 × 10−13 km s−12 from Begeman, Broeils, & Sanders 1991; (dotted line) and the best‐fit value (see Table 7; continuous line). Filled circles represent the data used in the fits (H I + Hα for NGC 3109 and 5585 and H I only for IC 2574 and NGC 3198). Open circles indicate Hα velocities not used in the fits.

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