Rotational studies in the Orion Nebula Cluster: from solar mass stars to brown dwarfs

M. V. Rodríguez-Ledesma; R. Mundt; J. Eislöffel

doi:10.1051/0004-6361/200811427

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Volume 502 / No 3 (August II 2009)

A&A, 502 3 (2009) 883-904

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Table 3:

Number of variable objects found in the ONC ( $\sim$ 1 Myr) by this study and in NGC 2264 ( $\sim$ 2 Myr) by L2004.
VarFlag^a	ONC ( $\sim$ 1 Myr)			NGC 2264 ( $\sim$ 2 Myr)
	$R< R_{\rm cluster}$	$R > R_{\rm cluster}$	Total	Total
PV	196	291	487	405
IV	335	473	808	184
All stars	847	2061	2908	10554

^a As in Table 1, PV are periodic variables and IV irregular variables. All stars include the total number of monitored stars independently of whether they are variables or not.

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