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| Query : 2011MNRAS.415.3771L |
2011MNRAS.415.3771L - Mon. Not. R. Astron. Soc., 415, 3771-3782 (2011/August-3)
Dissecting the colour–magnitude diagram: a homogeneous catalogue of stellar populations in globular clusters.
LEIGH N., SILLS A. and KNIGGE C.
Abstract (from CDS):
We have confirmed our previous result that there is a clear, but sublinear, correlation between the number of blue stragglers found in the cluster core and the total stellar mass contained within it. By considering a larger spatial extent than just the core, our results suggest that mass segregation is not the dominant effect contributing to the observed sublinearity. We also investigate the radial distributions of the different stellar populations in our sample of clusters. Our results are consistent with a linear relationship between the number of stars in these populations and the total mass enclosed within the same radius. Therefore, we conclude that the cluster dynamics does not significantly affect the relative distributions of these populations in our sample.
Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS
Journal keyword(s): catalogues - blue stragglers - stars: statistics - globular clusters: general
Simbad objects: 35
| Number of rows : 35 |
| 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 | NGC 188 | OpC | 00 47 14.8 | +85 14 42 | ~ | 990 | 0 | |||||
| 3 | NGC 1261 | GlC | 03 12 16.21 | -55 12 58.4 | 8.63 | ~ | 579 | 0 | ||||
| 4 | NGC 1851 | GlC | 05 14 06.76 | -40 02 47.6 | ~ | 1529 | 0 | |||||
| 5 | NGC 2298 | GlC | 06 48 59.41 | -36 00 19.1 | 8.89 | ~ | 547 | 0 | ||||
| 6 | NGC 3201 | GlC | 10 17 36.82 | -46 24 44.9 | ~ | 1001 | 0 | |||||
| 7 | NGC 4147 | GlC | 12 10 06.149 | +18 32 31.78 | 11.45 | 10.74 | ~ | 616 | 0 | |||
| 8 | M 68 | GlC | 12 39 27.98 | -26 44 38.6 | 7.96 | ~ | 1069 | 0 | ||||
| 9 | M 53 | GlC | 13 12 55.25 | +18 10 05.4 | 7.79 | ~ | 907 | 0 | ||||
| 10 | NGC 5139 | GlC | 13 26 47.28 | -47 28 46.1 | ~ | 3677 | 0 | |||||
| 11 | M 3 | GlC | 13 42 11.62 | +28 22 38.2 | 6.39 | ~ | 2593 | 0 | ||||
| 12 | NGC 5286 | GlC | 13 46 26.81 | -51 22 27.3 | ~ | 485 | 0 | |||||
| 13 | NGC 5466 | GlC | 14 05 27.29 | +28 32 04.0 | 9.70 | ~ | 887 | 0 | ||||
| 14 | M 5 | GlC | 15 18 33.22 | +02 04 51.7 | 5.95 | ~ | 2095 | 0 | ||||
| 15 | NGC 5927 | GlC | 15 28 00.69 | -50 40 22.9 | ~ | 499 | 0 | |||||
| 16 | NGC 5986 | GlC | 15 46 03.00 | -37 47 11.1 | 6.92 | ~ | 408 | 0 | ||||
| 17 | M 80 | GlC | 16 17 02.41 | -22 58 33.9 | ~ | 780 | 0 | |||||
| 18 | M 4 | GlC | 16 23 35.22 | -26 31 32.7 | ~ | 1978 | 0 | |||||
| 19 | NGC 6101 | GlC | 16 25 48.12 | -72 12 07.9 | ~ | 337 | 0 | |||||
| 20 | M 107 | GlC | 16 32 31.86 | -13 03 13.6 | ~ | 835 | 0 | |||||
| 21 | M 13 | GlC | 16 41 41.634 | +36 27 40.75 | 5.8 | ~ | 2291 | 0 | ||||
| 22 | M 12 | GlC | 16 47 14.18 | -01 56 54.7 | 6.07 | ~ | 736 | 0 | ||||
| 23 | M 10 | GlC | 16 57 09.05 | -04 06 01.1 | 4.98 | ~ | 857 | 0 | ||||
| 24 | M 92 | GlC | 17 17 07.39 | +43 08 09.4 | 6.52 | ~ | 2240 | 0 | ||||
| 25 | NGC 6362 | GlC | 17 31 54.99 | -67 02 54.0 | ~ | 637 | 0 | |||||
| 26 | NGC 6535 | GlC | 18 03 50.51 | -00 17 51.5 | 9.85 | ~ | 320 | 0 | ||||
| 27 | NGC 6584 | GlC | 18 18 37.60 | -52 12 56.8 | 8.17 | ~ | 317 | 0 | ||||
| 28 | M 69 | GlC | 18 31 23.10 | -32 20 53.1 | ~ | 492 | 0 | |||||
| 29 | NGC 6652 | GlC | 18 35 45.63 | -32 59 26.6 | ~ | 474 | 0 | |||||
| 30 | NGC 6723 | GlC | 18 59 33.15 | -36 37 56.1 | ~ | 543 | 0 | |||||
| 31 | M 56 | GlC | 19 16 35.57 | +30 11 00.5 | ~ | 455 | 0 | |||||
| 32 | M 71 | GlC | 19 53 46.49 | +18 46 45.1 | ~ | 1190 | 0 | |||||
| 33 | NGC 6934 | GlC | 20 34 11.37 | +07 24 16.1 | ~ | 459 | 0 | |||||
| 34 | M 72 | GlC | 20 53 27.70 | -12 32 14.3 | 8.96 | ~ | 465 | 0 | ||||
| 35 | M 2 | GlC | 21 33 27.02 | -00 49 23.7 | 6.25 | ~ | 1114 | 1 |
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