Figure 15 from The Next Generation Virgo Cluster Survey. V. Modeling the Dynamics of M87 with the Made-to-measure Method

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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 15.

Total mass-to-light ratio (in units of ) profile of NGC 4374. The dark blue solid and dashed lines are the total mass-to-light ratio profile of the minimum ΔG model and its uncertainty. The orange solid and dashed lines are the stellar M/L_V and uncertainty. The gray and red dashed regions are the corresponding total and stellar mass-to-light ratios of Napolitano et al. (2011).

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