&fortin 

  mass_P = 0.60
  mass_S = -1.0

  problem = 2

  tde_separation = 8.0d0
  tde_beta = 6.0d0

  interp_temp = T

  ambient_density = 1.0d-4

  stellar_temp = 1.0d7
  ambient_temp = 1.0d7

  max_stellar_tagging_level = 20
  max_temperature_tagging_level = 0
  max_center_tagging_level = 0
  stellar_density_threshold = 1.0d0
  temperature_tagging_threshold = 5.0d8
  center_tagging_radius = 0.0d0
  max_tagging_radius = 0.75d0
  roche_tagging_factor = 2.0d0

  center_fracx = 0.5d0
  center_fracy = 0.5d0
  center_fracz = 0.5d0

  initial_model_dx = 6.25d5	
  initial_model_npts = 4096
  initial_model_mass_tol = 1.d-6
  initial_model_hse_tol = 1.d-10

/

&tagging 

  ! Limit zone size based on nuclear burning considerations
  dxnuc_min = 0.1


/

&sponge

  sponge_lower_radius  = 0.0d0
  sponge_upper_radius  = 0.0d0
  sponge_lower_density = 1.0d0
  sponge_upper_density = 1.0d0
  sponge_timescale     = 0.01d0

/

&extern

  ! Note that some of the parameters in this
  ! namelist are specific to the default EOS,
  ! network, and/or integrator used in the 
  ! makefile. If you try a different set of 
  ! microphysics routines be sure to check that
  ! the parameters in here are consistent, as
  ! Fortran does not like seeing unknown variables
  ! in the namelist.

  small_x = 1.d-12

  use_eos_coulomb = T
  eos_input_is_constant = T

  burning_mode = 1

  do_constant_volume_burn = T
  call_eos_in_rhs = T

  rtol_spec = 1.d-6
  atol_spec = 1.d-6

  rtol_temp = 1.d-6
  atol_temp = 1.d-6

  rtol_enuc = 1.d-6
  atol_enuc = 1.d-6

  retry_burn = T

  renormalize_abundances = T

  MAX_TEMP = 1.d10

  ! Note that not every network has tabular
  ! rates enabled, so for some networks the
  ! following option will have no effect.

  use_tables = T

/