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DIFFERENTIAL REDDENING IN THE YOUNG CLUSTER NGC 2264
Publications of the Astronomical Society of the Pacific
Vol. 90, No. 534 (April 1978), pp. 144-148
Published by: Astronomical Society of the Pacific
Stable URL: http://www.jstor.org/stable/40677135
Page Count: 5
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A study of intermediate dispersion spectra, and broad-band photometry of 69 stars in the very young cluster NGC 2264 reveals the presence of extensive differential reddening. Statistical inquiries lead to the inference that the source of the reddening is intracluster dust clouds, but that these clouds may not be randomly distributed within the cluster.
Publications of the Astronomical Society of the Pacific © 1978 The University of Chicago Press