Universality of young cluster sequences | Astronomy & Astrophysics (A&A)

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Table A.2:

Properties of embedded clusters containing more than 200 observed stars.
Identification	distances	$M_{\rm c}$	Size	log ( $\rho_{\rm c}$ )
	[pc]	[ $M_{\odot }$ ]	[pc]	[ $M_{\odot }$ pc^-3]
02232 + 6138¹	2.4	130	0.91	2.23
02575 + 6017¹	2.4	150	1	2.17
IC 348¹	0.32	160	1	2.20
ONC ¹	0.45	1100	3.8	1.30
NGC 2024 ¹	0.4	180	0.88	2.42
MonR2 ¹	0.8	340	1.85	1.72

¹ Lada & Lada (2003), and references therein.

Source LaTeX | All tables | In the text

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