Line Emission Sources¶
LineSourceModel
assumes that the emission is
occuring at a single energy, and that it may or may not be broadened by thermal
or other motions. In the former case, the emission is a delta function at a
single rest-frame energy \(E_0\):
In the latter case, the emission is represented by a Gaussian with mean \(E_0\) and standard deviation \(\sigma_E\):
When creating a LineSourceModel
, it is
initialized with the line rest-frame energy e0
and an emission_field
field specification that represents the normalization \(A\) in the equations
above, which must be in units of counts/s. Optionally, the line may be broadened
by passing in a sigma
parameter, which can be a field specification or
YTQuantity
, corresponding to either a spatially varying field or a single
constant value. In either case, sigma
may have units of energy or velocity;
if the latter, it will be converted to a broadening in energy units via
\(\sigma_E = \sigma_v\frac{E_0}{c}\).
Note
In most cases, you will want velocity broadening of lines to be handled by
the inputted velocity fields instead of by the sigma
parameter. This
parameter is designed for thermal or other sources of “intrinsic”
broadening.
Examples¶
An example of an unbroadened line:
e0 = YTQuantity(5.0, "keV") # Rest-frame line energy
emission_field = ("gas", "line_emission") # Line emission field (normalization)
line_model = pyxsim.LineSourceModel(e0, line_emission)
An example of a line with a constant broadening in km/s:
e0 = YTQuantity(6.0, "keV")
emission_field = ("gas", "line_emission") # Line emission field (normalization)
sigma = (500., "km/s")
line_model = pyxsim.LineSourceModel(e0, line_emission, sigma=sigma)
An example of a line with a spatially varying broadening field:
e0 = YTQuantity(6.0, "keV")
emission_field = ("gas", "line_emission") # Line emission field (normalization)
sigma = "dark_matter_velocity_dispersion" # Has dimensions of velocity
line_model = pyxsim.LineSourceModel(e0, line_emission, sigma=sigma)