YusifovKucuk2004B¶
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class
gammapy.astro.population.YusifovKucuk2004B(amplitude=1, a=4, b=6.8, **kwargs)[source]¶ Bases:
astropy.modeling.Fittable1DModelRadial distribution of the surface density of OB stars in the galaxy - Yusifov & Kucuk 2004.
\[f(r) = A \left( \frac{r}{r_{\odot}} \right) ^ a \exp \left[ -b \left( \frac{r}{r_{\odot}} \right) \right]\]Derived empirically from OB-stars distribution.
Reference: http://adsabs.harvard.edu/abs/2004A%26A...422..545Y (Formula (17))
Parameters: amplitude : float
See model formula
a : float
See model formula
b : float
See model formula
See also
CaseBattacharya1998,Paczynski1990,YusifovKucuk2004,Lorimer2006,FaucherKaspi2006,ExponentialAttributes Summary
aamplitudebevolvedparam_namesMethods Summary
evaluate(r, amplitude, a, b)One dimensional Yusifov & Kucuk 2004 model function Attributes Documentation
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a¶
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amplitude¶
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b¶
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evolved= False¶
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param_names= ('amplitude', 'a', 'b')¶
Methods Documentation
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