A study of the interplay between ionized gas and star clusters in the central region of NGC 5253 with 2D spectroscopy

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Table 4:

Ages of the clusters associated with the W-R regions according to different indicators.
	Harris et al. (2004)		This work
Region	Clusters	Age	$\log$ (WR/(WR+O))	Age $_{\rm WR/O}$	EW(H $\beta$ )	Age $_{\rm H\beta}$
	Number	(Myr)		(Myr)	(Å)	(Myr)
Nucleus	1	3	-1.99	2.9	245	2.7
H II-2	20	3	-1.93	2.9	320	2.4
W-R 1	13	4	-1.34	3.2/4.8	131	3.4
W-R 2	23	5	-1.64	3.0/5.5	180	3.2
W-R 3	4, 24, 25	1-5	-1.55	3.0/5.3	128	3.4
W-R 4	6, 21	4	-1.35	3.2/4.8	131	3.4
W-R 5	...	...	-1.17	3.4	86	4.7

Source LaTeX | All tables | In the text

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