2006MmSAI..77..864C


Query : 2006MmSAI..77..864C

2006MmSAI..77..864C - Mem. Soc. Astron. Ital., 77, 864-868 (2006)

Are there radical cyanogen abundance differences between galactic globular cluster RGB and AGB stars? Possibly a vital clue to the globular cluster abundance anomaly problem.

CAMPBELL S.W., LATTANZIO J.C. and ELLIOTT L.M.

Journal keyword(s):

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 104 GlC 00 24 05.359 -72 04 53.20     4.09     ~ 4158 0
2 M 5 GlC 15 18 33.22 +02 04 51.7     5.95     ~ 2095 0
3 M 4 GlC 16 23 35.22 -26 31 32.7           ~ 1978 0
4 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
5 M 55 GlC 19 39 59.71 -30 57 53.1     6.49     ~ 913 0
6 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3274 0

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