The effect of ram pressure on the star formation, mass distribution and morphology of galaxies

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Volume 499 / No 1 (May III 2009)

A&A, 499 1 (2009) 87-102

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Table 2:

The properties of the ram pressure and the surrounding gas of the simulations.
	$v_{\rm {rel}}$	$\rho_{\rm {sur}}$	particle	p
run	[km s^-1]	[g/cm³]	number	[dyn cm^-2]
1	1000	$1\times10^{-28}$	$1.08\times10^{6}$	$1.00\times10^{-12}$
2	1000	$5\times10^{-28}$	$5.40\times10^{6}$	$5.00\times10^{-12}$
3	1000	$1\times10^{-27}$	$1.08\times10^{7}$	$1.00\times10^{-11}$
4	1000	$5\times10^{-27}$	$5.40\times10^{7}$	$5.00\times10^{-11}$
5	500	$1\times10^{-28}$	$1.08\times10^{6}$	$2.50\times10^{-13}$
6	500	$5\times10^{-28}$	$5.40\times10^{6}$	$1.25\times10^{-12}$
7	500	$1\times10^{-27}$	$1.08\times10^{7}$	$2.50\times10^{-12}$
8	500	$5\times10^{-27}$	$5.40\times10^{7}$	$1.25\times10^{-11}$
9	100	$1\times10^{-28}$	$1.08\times10^{6}$	$1.00\times10^{-14}$
10	100	$5\times10^{-28}$	$5.40\times10^{6}$	$5.00\times10^{-14}$
11	100	$1\times10^{-27}$	$1.08\times10^{7}$	$1.00\times10^{-13}$
12	100	$5\times10^{-27}$	$5.40\times10^{7}$	$5.00\times10^{-13}$

$v_{\rm {rel}}$ : relative velocity between the surrounding gas and the galaxy;
$\rho_{\rm {sur}}$ : surrounding gas density; p: ram pressure on the galaxy.

Source LaTeX | All tables | In the text

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