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

Authors: M. V. Rodríguez-Ledesma, R. Mundt and J. Eislöffel.<br />Astronomy and Astrophysics Vol. 515 , page A13<br />Published online: 31/05/2010<br />
Keywords:
stars: low-mass ; starts: pre-main sequence ; stars: rotation ; techniques: photometric ; brown dwarfs ; accretion, accretion disks.

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