This article has an erratum: [erratum]

A&A 380, 590-598 (2001)
DOI: 10.1051/0004-6361:20011461

New neighbours: IV. 30 DENIS late-M dwarfs between 15 and 30 parsecs

N. Phan-Bao^{1, 2}, J. Guibert^{1, 2}, F. Crifo², X. Delfosse³, T. Forveille^{3, 4}, J. Borsenberger⁵, N. Epchtein⁶, P. Fouqué^{7, 8} and G. Simon<sup>2

1</sup>  Centre d'Analyse des Images, DASGAL, Observatoire de Paris, 61 avenue de l'Observatoire, 75014 Paris, France
²  Observatoire de Paris (DASGAL/UMR-8633), 75014 Paris, France
³  Laboratoire d'Astrophysique de Grenoble, Université J. Fourier, BP 53, 38041 Grenoble, France
⁴  Canada-France-Hawaii Telescope Corporation, 65-1238 Mamalahoa Highway, Kamuela, HI 96743, USA
⁵  Institut d'Astrophysique de Paris, 98bis boulevard Arago, 75014 Paris
⁶  Observatoire de la Côte d'Azur, Département Fresnel, BP 4229, 06304 Nice Cedex 4, France
⁷  DESPA, Observatoire de Paris, 5 place J. Janssen, 92195 Meudon Cedex, France
⁸  European Southern Observatory, Casilla 19001, Santiago 19, Chile

(Received 16 July 2001 / Accepted 15 October 2001 )

Erratum

Abstract
We present 30 new nearby (d< 30 pc) red dwarf candidates, with estimated spectral types M 6 to M 8. 26 were directly selected from the DENIS database, and another 4 were first extracted from the LHS catalogue and cross-identified with a DENIS counterpart. Their proper motions were measured on the MAMA measuring machine from plates spanning 13 to 48 years, and are larger than 0.1 yr-1, ruling out the possibility that they are giants. Their distances were estimated from the DENIS colours and IR colour-magnitude relations and range between 15 and 30 pc.

Key words: astrometry -- proper motions -- low mass stars

Offprint request: N. Phan-Bao, bn.phan@obspm.fr

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© ESO 2001

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