Star formation in the intragroup medium and other diagnostics of the evolutionary stages of compact groups of galaxies

S. Torres-Flores; C. Mendes de Oliveira; D. F. de Mello; P. Amram; H. Plana; B. Epinat; J. Iglesias-Páramo

doi:10.1051/0004-6361/200911878

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Volume 507 / No 2 (November IV 2009)

A&A, 507 2 (2009) 723-746

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Table 8:

Observed and derived properties for HCG 100 regions.
ID	ID^a	RA	Dec	FUV	NUV	FUV-NUV^b	Age^c
		(2000)	(2000)				(Myr)
1	...	0.37526	13.16465	21.90 $\pm$ 0.10	21.38 $\pm$ 0.06	0.47 $\pm$ 0.10
2	...	0.30563	13.17565	21.70 $\pm$ 0.08	20.29 $\pm$ 0.03	0.81 $\pm$ 0.07
3	...	0.34740	13.16286	21.34 $\pm$ 0.07	20.31 $\pm$ 0.04	0.82 $\pm$ 0.09
4^d	4^d	0.29263	13.08581	21.39 $\pm$ 0.09	20.95 $\pm$ 0.07	0.00 $\pm$ 0.10	21.49
5	...	0.30592	13.14859	21.79 $\pm$ 0.11	20.70 $\pm$ 0.06	0.91 $\pm$ 0.12
6	6	0.30766	13.16278	20.38 $\pm$ 0.05	19.92 $\pm$ 0.03	0.23 $\pm$ 0.06
7	13	0.37282	13.09862	19.65 $\pm$ 0.03	19.19 $\pm$ 0.02	0.07 $\pm$ 0.05	48.75
8	14	0.37734	13.10402	21.51 $\pm$ 0.08	21.12 $\pm$ 0.07	-0.06 $\pm$ 0.08	10.86
...	3^d	0.27220	13.02360	21.21 $\pm$ 0.09	21.61 $\pm$ 0.08	-0.40 $\pm$ 0.12	<1

^a ID in de Mello et al. (2008a); ^b using a fixed aperture of 4 $^{\prime\prime}$ ; ^c age from FUV-NUV using Thilker et al. (2007); ^d recently obtained spectroscopy confirms these regions as part of HCG 100 (Urrutia-Viscarra et al. 2009).

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