vice.singlezone.MgSchmidt
=========================

Type : real number

Default : 6.0e+09

The normalization of the gas supply in :math:`M_\odot` when star
formation efficiency is dependent on the gas supply:

.. math:: \tau_\star \sim
	\left(\frac{M_g}{M_{g,\text{Schmidt}}}\right)^{-\alpha}

where :math:`\alpha` is specified by the attribute ``schmidt_index``.

.. note:: This attribute is irrelevant when the attribute ``tau_star``
	is a function of two variables.

.. tip::

	In practice, this quantity should be comparable to a typical gas
	supply of the simulated zone so that the actual star formation
	efficiency at a given timestep is near the user-specified value.

.. seealso::
	- vice.singlezone.tau_star
	- vice.singlezone.schmidt
	- vice.singlezone.schmidt_index

Example Code
------------
>>> import vice
>>> sz = vice.singlezone(name = "example")
>>> sz.MgSchmidt = 5.0e+09