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Issue A&A
Volume 457, Number 3, October III 2006
Page(s) L29 - L32
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:20065946



A&A 457, L29-L32 (2006)
DOI: 10.1051/0004-6361:20065946

Letter

2.3 $\mu$m CO emission and absorption from young high-mass stars in M 17

V. H. Hoffmeister1, R. Chini1, C. M. Scheyda1, D. Nürnberger2, N. Vogt3, 4 and M. Nielbock1

1  Astronomisches Institut, Ruhr-Universität Bochum, 44780 Bochum, Germany
    e-mail: vhoff@astro.rub.de
2  European Southern Observatory, Santiago 19, Chile
3  Instituto de Astronomía, Universidad Católica del Norte, Antofagasta, Chile
4  Departamento de Física y Meteorología, Universidad de Valparaíso, Chile

(Received 30 June 2006 / Accepted 25 July 2006)

Abstract
Aims.We are studying the extremely young cluster of M 17 to investigate the birth of high-mass stars and the initial mass function.
Methods.Deep ${\it JHKL}$ imaging and K-band spectroscopy from the VLT of 201 stars toward the cluster is presented.
Results.The majority of 104 stars show the CO band-head in absorption. Half of them emit X-rays and/or have infrared excess, indicative of very young objects. Their intrinsic IR luminosity is compatible with intermediate and high-mass pre-main sequence stars. Nine additional stars have the CO feature in emission, while sixty sources are lacking any stellar spectral feature due to veiling by circumstellar dust.
Conclusions.We suggest that CO absorption is - as in the case of low-mass stars - also a common feature during the early evolution of stars with higher masses. According to model calculations the observed CO absorption is most likely a sign of heavily accreting protostars with mass accretion rates above $10^{-5}~M_\odot$ yr-1.


Key words: infrared: stars -- ISM: $\ion{H}{ii}$ regions -- Galaxy: open clusters and associations: individual: M 17 -- Galaxy: open clusters and associations: individual: NGC 6618 -- stars: early-type -- stars: circumstellar matter



© ESO 2006

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