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On the highly reddened members in six young galactic star clusters: A multiwavelength study

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dc.contributor.author Kumar, B.
dc.contributor.author Sagar, R.
dc.contributor.author Sanwal, B. B.
dc.contributor.author Bessell, M. S.
dc.date.accessioned 2009-08-06T06:57:50Z
dc.date.available 2009-08-06T06:57:50Z
dc.date.issued 2004
dc.identifier.uri http://hdl.handle.net/123456789/228
dc.description.abstract The spectral and reddening properties of 211 highly reddened proper-motion members with V<15 mag in six young galactic star clusters are investigated using low-resolution spectroscopic, broad-band UBVRIJHK and mid-infrared (IR) data. We report emission features in Caɪɪ HK and Hɪ lines for a sample of 29 stars including 11 stars reported for the first time and also provide either a new or more reliable spectral class for a sample of 24 stars. Ca ɪɪ triple width measurements are used to indicate the presence of an accretion disc for a dozen stars and to indicate luminosity of couple of stars. On the basis of spectral features, near-IR excesses, dereddened colour-colour diagrams and mid-IR spectral indices we identify a group of 28 pre-main-sequence cluster members including five highly probable Herbig Ae/Be and six classical T Tauri stars. en_US
dc.language.iso en en_US
dc.relation.ispartofseries mn353-991
dc.subject Circumstellar Matter- Stars, Star Formation, Open Cluster en_US
dc.title On the highly reddened members in six young galactic star clusters: A multiwavelength study en_US
dc.type Article en_US


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