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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 1.

Top: the normalized surface density profiles. The black line is the GC surface number density profile along projected radius from Peng et al. (2008), the red solid and dashed lines are the stellar surface brightness profile along major and minor axis constructed from the M87 MGE in Cappellari et al. (2006), the purple solid and dashed lines are the g band surface brightness profile along major and minor axis from NGVS (L. Ferrarese et al., in preparation). The total luminosity/number for each profile within 80 kpc have been normalized to be unity. Bottom: the minor to major axis ratio q of the GC surface number density, Cappellari et al. (2006) and NGVS stellar surface brightness, respectively.

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