Star complexes and stellar populations in NGC 6822 - Comparison with the Magellanic Clouds

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Table 4:

Colour, magnitude and age limits and dominant stellar component of the selected colour-magnitude diagram regions.
Selected	V	(B-V)₀	age	Stellar
Region	(mag)	(mag)	(Myr)	Content
I	18.0-23.0	-0.4-0.0	$\leq$ 320	MS^a
II	23.0-24.0	-0.4-0.3	$\leq$ 630	MS^a
III	18.0-23.0	0.0-0.3	60-400	Post MS^b
IV	15.5-19.5	0.4-0.8	10-80	MW stars^c
V	19.5-22.0	0.4-0.8	80-320	Post MS^b
VI	22.0-24.0	0.4-0.8	320-500	Post MS^b
VII	19.0-20.5	1.3-1.6	130-630	MW stars^c
VIII	20.5-21.5	1.3-1.6	630-3160	MW stars^c
IX	21.5-24.0	1.0-2.0	$\geq$ 790	RGs^d

^a: Main Sequence stars.
^b: Post Main Sequence stars.
^c: Mostly Milky Way stars. The age range in Col. 4 is referring to NGC 6822 stars.
^d: Red Giants.

Source LaTeX | All tables | In the text

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