Differences

This shows you the differences between two versions of the page.

--- tests:streams [2015/09/02 13:30] – aspagna
+++ tests:streams [2022/10/24 12:10] (current) – external edit 127.0.0.1
@@ Line 84: / Line 84: @@
 We provide three catalogs based on high-resolution N-body simulations of the interaction between a
-Milky-Way like galaxy and orbiting dwarf galaxies with four representative cases of merging histories in term of dynamical friction properties (see [[ftp://ftp.oato.inaf.it/astrometria/paola/InnerHaloModel/mergingsatellites_4.6Gyr.jpg|figure]]).
+Milky-Way like disk galaxy within a dark matter halo and orbiting dwarf galaxies with four representative cases of merging histories in term of dynamical friction properties (see [[ftp://ftp.oato.inaf.it/astrometria/paola/InnerHaloModel/mergingsatellites_4.6Gyr.jpg|figure]]).
 These catalogs include the 3D position and 3D velocities of the accreted particles within 3 kpc of the Sun after 4.63 Gyr:
@@ Line 104: / Line 104: @@
      id=1  local smooth halo (mock catalog)
-Further details on this data set are given in [[http://adsabs.harvard.edu/abs/2015arXiv150803736R|Re Fiorentin et al. (2015)]].
+Further details are given in [[http://adsabs.harvard.edu/abs/2015arXiv150803736R|Re Fiorentin et al. (2015)]].  The N-body simulations are from [[http://adsabs.harvard.edu/abs/2010ApJ...716L.115M | Murante et al. 2010]].
 For any questions please feel free to contact Alessandro Spagna (spagna@oato.inaf.it) or Paola Re Fiorentin (re_fiorentin@oato.inaf.it).