Available formats: HTML | PDF | (gzipped) PostScript
L. Deharveng 1,
A. Zavagno 1,
D. Nadeau 2,
J. Caplan 1 and
M. Petit 1
Received 28 July 1998 / Accepted 14 January 1999
We present a photometric and spectroscopic study of the compact H II region Sh 138 and its associated stellar cluster. The positions and BVRIJHK magnitudes are obtained for more than 400 stars over a field of about 4´ square centred on the H II region. Sh 138 is excited by a cluster of young massive stars. At the cluster's very centre are at least four O-B2 stars separated by less than 4". The brightest of these, both in the visible and the near infrared, exhibits a spectrum similar to those of the more massive Herbig Ae/Be stars. This star, our No. 183, is overluminous by a factor of 2.5 in the visible and four in the near IR with respect to the O9.5 V star required to account for the ionization level of the H II region. However star 183's position in the versus diagram does not indicate a near-IR excess. We suggest that this star is a young massive object belonging to a binary or multiple system.
The stellar cluster associated with Sh 138 is very reminiscent of the Orion Trapezium cluster: it is centrally peaked around several massive stars, and is dense - more than 550 stars pc-2 at its centre. The visual extinction in the cluster varies between 5 mag and more than 35 mag; large variations are observed over very small scales (for example, more than 20 mag over less than 4" among the central massive stars).
Key words: stars: pre-main sequence ISM: H ii regions ISM: individual objects: Sh 138 Galaxy: open clusters and associations: individual: Sh 138 infrared: stars
* Based on observations done at the Observatoire de Haute Provence and the Observatoire du Pic du Midi, France, and at the Canada-France-Hawaii Telescope. The CFHT is operated by the Centre National de la Recherche Scientifique of France, the National Research Council of Canada and the University of Hawaii.
Send offprint requests to: L. Deharveng
Online publication: March 29, 1999