Abstract
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 13 m. 50 and its earliest spectral type is BO.
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© 1984 D. Reidei Publishing Company
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Hassan, S.M. (1984). The Young Open Cluster NGC 2384. In: Capaccioli, M. (eds) Astronomy with Schmidt-Type Telescopes. Astrophysics and Space Science Library, vol 110. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6387-0_50
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DOI: https://doi.org/10.1007/978-94-009-6387-0_50
Publisher Name: Springer, Dordrecht
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