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A&A 462, 157-162 (2007)
DOI: 10.1051/0004-6361:20065513
Investigating star formation in the young open cluster NGC 6383
E. Paunzen, M. Netopil, and K. ZwintzInstitut für Astronomie der Universität Wien, Türkenschanzstr 17, 1180 Wien, Austria
e-mail: Ernst.Paunzen@univie.ac.at
(Received 26 April 2006 / Accepted 18 October 2006)
Abstract
Context.By studying young open clusters, the mechanisms important for
star formation over several Myr can be examined. For example, accretion
rate as a function of rotational velocity can be investigated. Similarly, sequential star formation
triggered by massive stars with high mass-loss rates can be studied in detail.
Aims. We identified and characterized probable members of NGC 6383, as well as determined cluster parameters.
Methods. New Strömgren uvby CCD photometry, obtained by us, is presented. This new data,
together with Johnson UBV and 2MASS data in the
NIR, was used to investigate characteristics of pre- as well as zero age main sequence cluster members.
Results. We present Strömgren uvby CCD photometry for 272 stars in the field of NGC 6383
and derive its reddening,
mag, as well as distance,
d = 1.7(3) kpc from the Sun. Several stars with NIR excess and objects in the
domain of the classical Herbig Ae/Be and T Tauri stars were detected. Two previously known
variables were identified as rapidly-rotating PMS stars. The field population is
clearly separated from the probable members in the color-magnitude diagram.
Conclusions. NGC 6383 is a young open cluster, with an age of less than 4 Myr, undergoing
continuous star formation. True pre-main sequence members might be found down
to absolute magnitudes of +6 mag, with a variety of rotational velocities
and stellar activities.
Key words: stars: pre-main sequence -- stars: early-type -- stars: formation -- open clusters and associations: individual: NGC 6383
© ESO 2007
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