old_contents: # Licensed under a 3-clause BSD style license - see LICENSE.rst
  
  """
  Project package for studying chaos in the Ophiuchus stream
  """
  
  # Affiliated packages may add whatever they like to this file, but
  # should keep this content at the top.
  # ----------------------------------------------------------------------------
  from ._astropy_init import *
  # ----------------------------------------------------------------------------
  
  # For egg_info test builds to pass, put package imports here.
  if not _ASTROPY_SETUP_:
      from .potential import OphiuchusPotential
  
      # These are the canonical potentials I'll use in the paper:
      #   - One Milky Way model with a time-dependent Bar
      #   - One axisymmetric, static Milky Way model
      barred_mw = OphiuchusPotential()
      static_mw = OphiuchusPotential(bar=dict(m=0.),
                                     spheroid=dict(m=1E10, c=0.2),
                                     disk=dict(m=6.E10))
  
new_contents: # Licensed under a 3-clause BSD style license - see LICENSE.rst
  
  """
  Project package for studying chaos in the Ophiuchus stream
  """
  
  # Affiliated packages may add whatever they like to this file, but
  # should keep this content at the top.
  # ----------------------------------------------------------------------------
  from ._astropy_init import *
  # ----------------------------------------------------------------------------
  
  # For egg_info test builds to pass, put package imports here.
  if not _ASTROPY_SETUP_:
      from .potential import OphiuchusPotential
  
      # These are the canonical potentials I'll use in the paper:
      #   - One Milky Way model with a time-dependent Bar
      #   - One axisymmetric, static Milky Way model
      barred_mw = OphiuchusPotential()
      static_mw = OphiuchusPotential(bar=dict(m=0.),
                                     spheroid=dict(m=1E10, c=0.2),
                                     disk=dict(m=6.5E10))
  
subject: change mass of disk