Palomar 8 / C1838-198 
(Updated July 2014)

RA: 18:41:29.9  DEC: -19:49:33 (J2000)

No known variables.
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Supplementary Notes 

Armandroff (1988) obtained CCD images in the V,R,I bands to compare the 
CM diagram of Pal 8 with that of 47 Tuc.  He found that the HB of Pal 8 
lies entirely redward of red edge of the instability strip, characteristic 
of a metal rich cluster.  It does not extend as far to the blue as the red 
HB of 47 Tuc.
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References

Armandroff, T. E. 1988, AJ, 96, 588 
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