2000NewAR..44..351P


Query : 2000NewAR..44..351P

2000NewAR..44..351P - New Astronomy Reviews, 44, 351-353 (2000)

Were the Old Halo globular clusters able to sustain a self-enrichment phase ?

PARMENTIER G., JEHIN E., MAGAIN P., NOELS A. and THOUL A.

Journal keyword(s):

Simbad objects: 8

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Number of rows : 8
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 288 GlC 00 52 45.24 -26 34 57.4   10 8.13     ~ 1130 0
2 NGC 362 GlC 01 03 14.26 -70 50 55.6     6.58     ~ 1167 0
3 M 3 GlC 13 42 11.62 +28 22 38.2     6.39     ~ 2593 0
4 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
5 M 54 GlC 18 55 03.33 -30 28 47.5           ~ 1164 0
6 Cl Terzan 7 GlC 19 17 43.92 -34 39 27.8           ~ 460 0
7 Cl Arp 2 GlC 19 28 44.11 -30 21 20.3     12.41     ~ 384 0
8 Cl Terzan 8 GlC 19 41 44.41 -33 59 58.1     11.54     ~ 357 0

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