Rotation-disk connection for very low mass and substellar objects in the Orion Nebula Cluster

Free Access

Table 4:

Median values of ptp amplitudes for objects with ( $\Delta(I-K)~+$ ) and without ( $\Delta(I-K)~-)$ IR excess.
	$R<R_{\rm cluster}$				$R>R_{\rm cluster}$				Whole WFI field
	$\Delta(I-K)+$		$\Delta(I-K)-$		$\Delta(I-K)+$		$\Delta(I-K)-$		$\Delta(I-K)+$		$\Delta(I-K)-$
Mass bins^a	B	C	B	C	B	C	B	C	B	C	B	C
N	44	8	97	8	48	22	150	35	93	30	243	43
$\langle PTP \rangle$ [mag]	0.12	0.24	0.05	0.16	0.11	0.23	0.03	0.08	0.12	0.24	0.04	0.1

Notes. ^(a) Mass bins as defined in Sect. 3: A is not shown due to the small sample number, B corresponds to the intermediate bin with $0.4<M <0.075~M_\odot$ and C to the faint bin in which all objects have $\textit{M}<0.075~M_\odot$ .

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.