Evidence of early disk-locking among low-mass members of the Orion Nebula Cluster (Corrigendum)

K. Biazzo; C. H. F. Melo; L. Pasquini; S. Randich; J. Bouvier; X. Delfosse

doi:doi:10.1051/0004-6361/200913125e

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This article is an erratum for: [this article]

Issue		A&A Volume 533, September 2011


Article Number		C3
Number of page(s)		1
Section		Galactic structure, stellar clusters and populations
DOI		http://dx.doi.org/10.1051/0004-6361/200913125e
Published online		16 September 2011

A&A 533, C3 (2011)

Evidence of early disk-locking among low-mass members of the Orion Nebula Cluster (Corrigendum)

K. Biazzo¹^,2^,3, C. H. F. Melo², L. Pasquini², S. Randich¹, J. Bouvier⁴ and X. Delfosse⁴

¹ INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
e-mail: kbiazzo@arcetri.astro.it
² ESO – European Southern Observatory, Karl-Schwarzschild-Str. 3, 85748 Garching bei München, Germany
³ INAF – Osservatorio Astrofisico di Catania, via S. Sofia 78, 95123 Catania, Italy
⁴ Laboratoire d’Astrophysique, Observatoire de Grenoble, BP 53, 38041 Grenoble Cedex 9, France

This article has no abstract.

Key words: open clusters and associations: individual: Orion Nebula Cluster / stars: low-mass / stars: pre-main sequence / stars: late-type / accretion, accretion disks / errata, addenda

Erratum of: A&A 508, 13011312 (2009), DOI: 10.1051/0004-6361/200913125

© ESO, 2011

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