&fortin 

  mass_P = 0.60
  mass_S = -1.0

  problem = 2

  tde_separation = 8.0d0
  tde_beta = 6.0d0

  nsub = 16

  max_stellar_tagging_level = 20
  max_temperature_tagging_level = 0
  stellar_density_threshold = 1.0d0

/

&ambient

  ambient_density = 1.0d-4
  ambient_temp = 1.0d7

/

&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

  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

  abort_on_failure = F
  retry_burn = F

  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

/