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STR#_532.txt
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1995-12-14
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119 lines
Linear diameter:
Distance above the formal galactic plane:
Galactocentric distance:
Magnitude of the brightest star:
Spectral class code:
Number of stars considered:
Integrated B-V:
Long period variable stars
marginal Ap stars
marginal Am stars
WR stars
U Geminorum stars
Shell stars
Planetary nebulae
Of stars
He weak stars
Delta Scuti stars
Cepheids
Carbon stars
Beta Cephei stars
Be+Shell stars
Be stars
Ba II stars
Ap stars
Am stars
Numbers of peculiar stars:
km/s
Radial velocity:
Metallicity, log (Fe/H) - log (Fe/H) for Sun:
years
Log(age) derived from turn-off color:
Turn-off color:
Reddening, E(B-V):
pc.
Distance:
Angular diameter:
Membership number:
Cluster is involved in nebulosity
bright and faint stars in the cluster
medium range in brightness
most stars of nearly the same brightness
Trumpler range of brightness:
very rich
rich
medium
poor
very poor
Trumpler richness:
not detached
detached, no concentration
detached, slight concentration
detached, strong concentration
Trumpler concentration class:
Galactic latitude:
Galactic longitude:
Galactic coordinates:
Lund number:
OCL number:
Other name: