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The Next Generation Virgo Cluster Survey. V. Modeling the Dynamics of M87 with the Made-to-measure Method

  • Authors: Ling Zhu, R. J. Long, Shude Mao, Eric W. Peng, Chengze Liu, Nelson Caldwell, Biao Li, John P. Blakeslee, Patrick Côté, Jean-Charles Cuillandre, Patrick Durrell, Eric Emsellem, Laura Ferrarese, Stephen Gwyn, Andrés Jordán, Ariane Lançon, Simona Mei, Roberto Muñoz, and Thomas Puzia

Zhu et al. 2014 The Astrophysical Journal 792 59.

  • Provider: AAS Journals

Caption: Figure 13.

Degeneracy of the scale velocity and scale radius in the logarithmic dark matter model. The insert panel enlarges the inner region marked by the dashed rectangle box. Each line represents a mass distribution of a logarithmic model. Dashed lines are models with VL = 650 km s−1, and solid lines are models with VS = 550 km s−1. Black indicates RL = 53 kpc and red indicates RS = 28.6 kpc. (The subscript S indicates "smaller" and L is "larger.")

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