Starbursts in isolated galaxies - I. The influence of stellar birth function and IMF

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Table 1:

Properties of the numerical models.
Model	SF-law (n, C_n, $T_{\rm s}$ )	Comment
A	1.5, 0.06, 10²	reference model
A2	1.5, 0.06, 10⁴
DN1	1.0, 0.007, $\infty$	no feedback, Schmidt law
DN2	1.1, 0.007, $\infty$
DN3	1.5, 0.007, $\infty$
DN4	2.0, 0.007, $\infty$
DN5	2.5, 0.007, $\infty$
DN6	2.0, 0.7, $\infty$	enhanced C_n
DT1	1.0, 0.007, 10⁵	with thermal feedback
DT2	1.0, 0.007, 10⁴
DT3	1.0, 0.007, 10³
DT4	1.0, 0.007, 10²
DT5	2.0, 0.55, 10⁵	quadr. Schmidt law with feedback
DI1	ind. SF only	induced star formation mode
DI2	model A, $T_{\rm s} = 10^2$	combined SF modes
DI3	model A, $T_{\rm s} = 10^4$	combined SF modes
DX1	model A, $\xi= 6\%$	varied constant IMF
DX2	model A, $\xi= 12\%$
DWK1	1.5, 0.06, 10²	Weidner-Kroupa IMF, SN heating
DWK2	1.5, 0.06, 10²	radiative heating

Source LaTeX | All tables | In the text

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