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The Young Open Cluster NGC 2384
Published online by Cambridge University Press: 12 April 2016
Abstract
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Combined photoelectric – photographic UBV-photometry for NGC 2384 is discussed. The results achieved so far are summarized and indicate that this cluster is young enough to be used as spiral arm tracer out to a distance of 3.27 kpc. The colour excess E(B-V) is 0.31, the apparent distance modulus is 13m.50 and its earliest spectral type is BO.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 78: Astronomy with Schmidt-type telescopes , 1984 , pp. 295 - 299
- Copyright
- Copyright © Reidel 1984
References
Schmidt-Kaler, Th., 1965, in Voigt, H.H. (ed.), Group VI/1, Springer-Verlag (Berlin), p.284
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