>> Interestingly, IC 348 is also known as IC 1985... From Harold Corwin's commentaries at the NGC/IC web site: IC 348 = IC 1985, which see. Dreyer put this into the first IC apparently without seeing Safford's footnote which reads, "A loose cluster with nebula." All that appears in the IC description is Safford's "vL, vgbM, pB" rearranged into the usual brightness-size-concentration order. Whatever happened, Safford is right -- there is a cluster associated with this nebulosity. Barnard did not mention the cluster, either, in his discovery note for IC 1985, though he examined the object both photographically and visually with the Yerkes 40-inch. IC 1985 = IC 348. Barnard did not check the first IC before he published this as a new nebula at the end of his paper on the "Exterior Nebulosities of the Pleiades." Dreyer apparently did not, either, so the object now has two IC numbers. See IC 348 for more. The nebulosity that caught Barnard's eye on a photograph of the Pleiades also contains a cluster, though the cluster is not visible on either of Barnard's photographs in his Lick Publications, Vol. 11. (Safford actually did see the cluster, though Dreyer did not put that into the description for IC 348.) The region is now, by the way, well-studied particularly for young low-mass stars. The classic study of the brighter stars was done in 1922 by Gingrich: 1922ApJ....56..139G GINGRICH C.H. Astrophys. J., 56, 139-144 (1922) Parallaxes of stars in the region of BD+31 643. The bright 'central star' HD 281159 = BD+31 643 is of spectral type B5V, so is not hot enough to fluoresce the gas, so this strictly a reflection nebula. The relatively reddish color is due to interestellar reddening between us and it. HD 281159 has B-V color about 0.8 mag redder than it would have if it were unobscured. \Brian -- See message header for info on list archives or unsubscribing, and please send personal replies to the author, not the list.