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The Extended H I Rotation Curve and Mass Distribution of M31

  • Authors: Claude Carignan, Laurent Chemin, Walter K. Huchtmeier, and Felix J. Lockman

Carignan et al. 2006 The Astrophysical Journal Letters 641 L109.

  • Provider: AAS Journals

Caption: Fig. 2.

Rotation curve and mass model for M31. The new rotation velocities from the Effelsberg and GBT 100 m observations are for ﹩R> 21﹩ kpc. The velocities for ﹩R\leq 21﹩ kpc are recomputed from the Unwin (1983) H I data. The upward‐pointing triangles (light gray) are for the receding side, and the downward‐pointing (dark gray) ones for the approaching side, as obtained from a tilted‐ring model (see text). The solid line is the best fit to the data. Each mass component is identified. A mass of ﹩1.0\times 10^{8}\,M_{\odot }﹩ is used for the central black hole (Bender et al. 2005).

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