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Sam Mangham edited this page Jul 25, 2019 · 3 revisions

KWD

KWD.mdot_r_exponent

The exponent for the mass loss rate as defined in the KWD model, m_dot(r) = F(r) ** alpha = T(r) ** (4 * alpha). F is the local luminous flux and T is the local temperature at a radius R. A value of 0 sets a uniform mass loss rate.

Type: Double

Values: Greater than or equal to 0

Parent(s):

File: knigge.c

KWD.v_zero

Multiple of the local sound speed at the base of the wind, this results in the initial velocity of the wind being able to be greater or less than the local sound speed.

Type: Double

Unit: Sound speed at wind base

Values: Greater than 0

Parent(s):

File: knigge.c

KWD.acceleration_length

The size of the acceleration length scale for a disk wind described by the KWD model.

Type: Double

Unit: cm

Values: Greater than 0

Parent(s):

File: knigge.c

KWD.rmax

The radius at which the disk wind terminates, in units of central object radii. This has to be greater than rmin.

Type: Double

Unit: :ref:`Central_object.radius`

Values: Greater than :ref:`KWD.rmin`

Parent(s):

File: knigge.c

KWD.acceleration_exponent

Sets the length scale over which the accleration to v_inf is accomplished. It is the value of the exponent beta for the Caster & Lamers equation of a stellar wind, v(r) = v_0 + (v_inf - v_0) * (1 - R_s/r) ** beta.

Type: Double

Values: Greater than 0

Parent(s):

File: knigge.c

KWD.rmin

The radius at which the disk wind begins, in units of central object radii.

Type: Double

Unit: :ref:`Central_object.radius`

Values: Greater than 1

Parent(s):

File: knigge.c

KWD.d

The ratio d/d_min is used to describe the degree of geometric collimation of the disk wind in the KWD model. However, d (the distance to the focal point in central object radii) is used as this provides a more natural parameter.

Type: Double

Unit: :ref:`Central_object.radius`

Values: Greater than 0

Parent(s):

File: knigge.c

KWD.v_infinity

The velocity at large distances of a steller wind described by the KWD model, in units of escape velocity. Described in terms of Castor & Lamers equation, v(r) = v_0 + (v_inf - v_0) * (1 - R_s/r) ** beta.

Type: Double

Unit: Escape velocity

Values: Greater than 0

Parent(s):

File: knigge.c

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