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Query : 2018ApJ...853..186Z |
2018ApJ...853..186Z - Astrophys. J., 853, 186-186 (2018/February-1)
No evidence of chemical abundance variations in the intermediate-age cluster NGC 1783.
ZHANG H., DE GRIJS R., LI C. and WU X.
Abstract (from CDS):
Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.
Journal keyword(s): galaxies: individual: Large Magellanic Cloud - globular clusters: individual: NGC 1783 - Hertzsprung-Russell and C-M diagrams - stars: abundances - stars: abundances
Simbad objects: 16
Number of rows : 16 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | ESO 28-19 | Cl* | 00 24 45.98 | -72 47 37.9 | 11.6 | 12.05 | ~ | 148 | 0 | |||
2 | NGC 121 | GlC | 00 26 49.0 | -71 32 10 | 11.2 | 11.24 | ~ | 310 | 0 | |||
3 | NAME SMC | G | 00 52 38.0 | -72 48 01 | 2.79 | 2.2 | ~ | 11142 | 1 | |||
4 | NGC 339 | OpC | 00 57 47.62 | -74 28 14.6 | 13.23 | 12.94 | 12.21 | 11.20 | ~ | 144 | 0 | |
5 | NGC 419 | OpC | 01 08 17.26 | -72 53 01.8 | 11.41 | 11.16 | 10.50 | 9.34 | ~ | 272 | 0 | |
6 | NAME Magellanic Clouds | GrG | 03 00 | -71.0 | ~ | 7059 | 0 | |||||
7 | NGC 1783 | GlC | 04 59 08.590 | -65 59 15.84 | 10.9 | 10.93 | ~ | 253 | 0 | |||
8 | NGC 1806 | GlC | 05 02 11.180 | -67 59 05.89 | 11.1 | ~ | 157 | 0 | ||||
9 | NGC 1846 | Cl* | 05 07 34.900 | -67 27 32.45 | 12.08 | 11.31 | ~ | 215 | 0 | |||
10 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 17424 | 0 | ||||
11 | NGC 1978 | GlC | 05 28 45.330 | -66 14 12.04 | 10.7 | 10.70 | ~ | 308 | 0 | |||
12 | NAME Hodge 4 | GlC | 05 32 25.64 | -64 44 07.7 | 13.33 | ~ | 49 | 0 | ||||
13 | ESO 86-22 | Cl* | 05 42 29.090 | -65 21 46.33 | 13.8 | ~ | 43 | 0 | ||||
14 | NGC 2121 | Cl* | 05 48 13.190 | -71 28 52.00 | 13.21 | 12.37 | ~ | 132 | 0 | |||
15 | NGC 2155 | Cl* | 05 58 32.070 | -65 28 38.62 | 13.41 | 12.60 | ~ | 106 | 0 | |||
16 | NGC 2193 | Cl* | 06 06 17.31 | -65 05 55.5 | 14.13 | 13.42 | ~ | 47 | 0 |
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