Imaging of star clusters in unperturbed spiral galaxies with the Advanced Camera for Surveys - II. A comparison of star cluster systems in five late type spirals

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Table 7:

Luminosity function coefficients.
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)
Galaxy	a	b	$\alpha$	$V_{\rm exp}$	$M_{v}^{\rm mean}$	$M_{v}^{\rm median}$	$\sigma_{\rm stoch}$	$V_{\rm obs}$	$\log{{\rm Mass}}$	$\log{{\rm Age}}$	Z
NGC 45¹	$0.37\pm0.11$	$-7.89 \pm0.37$	$-1.93\pm0.3$	$20.79\pm2.29$	18.63	18.93	1.57	20.697	2.97	6.66	0.004
NGC 1313	$0.43\pm0.04$	$-8.28 \pm0.87$	$-2.08\pm0.1$	$19.13\pm1.14$	17.08	17.26	1.15	15.856	5.22	6.60	0.008
NGC 4395	$0.29\pm0.01$	$-5.69 \pm1.7$	$-1.72\pm0.2$	$19.59\pm5.28$	16.43	16.74	1.93	19.541	3.97	7.08	0.02
NGC 5236	$0.55\pm0.04$	$-10.61\pm0.92$	$-2.38\pm0.11$	$19.22\pm1.06$	18.02	18.21	1.01	18.062	4.72	7.39	0.02
NGC 7793	$0.40\pm0.05$	$-7.60 \pm1.25$	$-1.99\pm0.13$	$19.41\pm2.13$	17.01	17.24	1.49	18.190	4.66	7.64	0.004

¹ From Mora et al. (2007)

Source LaTeX | All tables | In the text

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