The globular cluster system of NGC 1399 - V. dynamics of the cluster system out to 80 kpc

Y. Schuberth; T. Richtler; M. Hilker; B. Dirsch; L. P. Bassino; A. J. Romanowsky; L. Infante

doi:10.1051/0004-6361/200912482

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Volume 513 (April 2010)

A&A, 513 (2010) A52

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Table 5:

Globular cluster number density profiles.
	N₀	R₀	$\alpha$	$\mathcal{B}\left(\frac{1}{2},\alpha \right)$
	[ $\rm {GCs~ arcmin}^{-2}$ ]	[arcmin]
Red	28.43 $\pm$ 7.82	1.63 $\pm$ 0.34	1.02 $\pm$ 0.04	1.98
Blue	8.39 $\pm$ 1.05	2.91 $\pm$ 0.42	0.79 $\pm$ 0.03	2.32
All	35.54 $\pm$ 6.13	1.74 $\pm$ 0.27	0.84 $\pm$ 0.02	2.22

Notes. Fitting a cored power-law (Eq. (10)) to the data given in Table 2 of Bassino et al. (2006) yields the parameters listed above (the profile for ``all'' GCs was obtained by adding the number counts of the red and blue GCs).

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