The hydrodynamics of the supernova remnant Cassiopeia A - The influence of the progenitor evolution on the velocity structure and clumping

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Table 1:

Adopted progenitor star wind parameters for our Cas A hydrodynamic simulations: final evolutionary phase of the progenitor star, duration of this phase, corresponding mass loss rate and wind velocity, total amount of mass and kinetic energy lost during this phase, and model acronym.
	$\tau$ [yr]	$\dot{M}~[$ ${M}_{\odot}$ /yr]	v [km s^-1]	$\Delta M~[$ ${M}_{\odot}$ ]	$\Delta E~ [10^{45}~{\rm erg}]$	Model
Red Supergiant	$8.75 \times 10^5$	$1.54 \times 10^{-5}$	4.70	13.5	5.93	WR0
Wolf Rayet	$5 \times 10^3$	$9.72 \times 10^{-6}$	$1.716 \times 10^3$	0.05	$1.42 \times 10^3$	WR5
Wolf Rayet	$10 \times 10^3$	$9.72 \times 10^{-6}$	$1.716 \times 10^3$	0.10	$2.85 \times 10^3$	WR10
Wolf Rayet	$15 \times 10^3$	$9.72 \times 10^{-6}$	$1.716 \times 10^3$	0.15	$4.27 \times 10^3$	WR15

Source LaTeX | All tables | In the text

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