Aligned/combined all files in AutostarSuite Image Processing software
Imported resulting file to Photoshop 7 via FITS liberator
Adjusted levels and Curves a bit
Minor noise reduction via Noel Carboni's "Space Noise Reduction" photoshop action
Description: NGC 869 and NGC 884 - AKA "The Double Cluster"
Perhaps known pre-historically. Cataloged 130 B.C. by Hipparcos.
The famous double cluster in Perseus was known in antique times (probably even pre-historically), and first cataloged by the Greek astronomer Hipparcos.
Both clusters are situated in the Perseus OB 1 association, and also only a few hundred light-years appart, at a distance of over 7000 light years. They are both quite young: h is listed at 5.6, chi at 3.2 million years (Sky Catalog 2000); their hottest main sequence stars are of spectral type B0. They are approaching us at 22 (h) and 21 (chi) km/sec, respectively.
O'Meara and Green (2003) point out to some historical confusion about the identity of the designations or names, or the objects "Chi" and "h" Persei. As they point out, since the 1840s, the name "Chi" is attributed to NGC 884, and "h" to NGC 869. However, these authors point out that very probably, Tycho Brahe measured one position for the "nebulous star" that is actually the double cluster, and Johann Bayer designated this "star" as Chi. Probably, he used the name "h Persei" for a fainter nearby star.
