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Shell.autogen
The velocity of a shell wind at the inner edge of the shell - the variation of the velocity in the shell is set by the velocity law exponent. It allows a gradient to be enforced.
Type: Double
Unit: cm/s
Values: Greater than or equal to 0
Parent(s):
- :ref:`Wind.type`: shell
File: shell_wind.c
Multi-line description, must keep indentation.
Type: Double
Unit: cm
Values: Greater than :ref:`Shell.wind.radmin`
Parent(s):
- :ref:`Wind.type`: shell
File: shell_wind.c
The mass loss through a diagnostic shell type wind. One normally sets this experimentally in order to get a required hydrogen density in the shell
Type: Double
Unit: M☉/year
Values: Greater than 0
Parent(s):
- :ref:`Wind.type`: shell
File: shell_wind.c
The velocity of a shell wind at the outer edge of the shell - the variation of the velocity in the shell is set by the velocity law exponent. It allows a gradient to be enforced.
Type: Double
Unit: cm/s
Values: Greater than or equal to 0
Parent(s):
- :ref:`Wind.type`: shell
File: shell_wind.c
The innermost edge of a diagnostic type of wind made up of a single (ideally thin) shell.
Type: Double
Unit: cm
Values: Greater than 0
Parent(s):
- :ref:`Wind.type`: shell
File: shell_wind.c
Exponent beta for the Caster and Lamers description of a stellar wind v(r)=v_o + (v_inf - v_o) (1+R_s/r)**beta for a shell wind.
Type: Double
Values: Greater than or equal to 0
Parent(s):
- :ref:`Wind.type`: shell
File: shell_wind.c