2016MNRAS.458.4162M


Query : 2016MNRAS.458.4162M

2016MNRAS.458.4162M - Mon. Not. R. Astron. Soc., 458, 4162-4171 (2016/June-1)

Multiple stellar populations in the globular cluster M3 (NGC 5272): a Stromgren perspective.

MASSARI D., LAPENNA E., BRAGAGLIA A., DALESSANDRO E., CONTRERAS RAMOS R. and AMIGO P.

Abstract (from CDS):

We present Stromgren photometry of the Galactic Globular Cluster M3 to study its multiple generations phenomenon. The use of different colour-magnitude diagrams (CMDs) and especially of the notoriously efficient cy index allowed us to detect a double red giant branch in the cluster CMD. After decontamination from fore- and background sources, the two sequences turned out to be equally populated. The two components also show a bimodal radial distribution well corresponding to that predicted by numerical simulations for clusters living in an intermediate dynamical evolutive state and with a population with modified chemical composition that was born more centrally concentrated than the primordial. The analysis of high-resolution spectra quantitatively demonstrates that the two detected sequences correspond to the first (Na-poor) generation and the second (Na-rich) generation, thus confirming the importance of synergy between photometry and spectroscopy.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): techniques: photometric - stars: abundances - Hertzsprung-Russell and colour-magnitude diagrams - stars: Population II - globular clusters: general - globular clusters: individual: ngc5272

VizieR on-line data: <Available at CDS (J/MNRAS/458/4162): catalog.dat>

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 23

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Number of rows : 23
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 1851 GlC 05 14 06.76 -40 02 47.6           ~ 1529 0
3 NGC 2808 GlC 09 12 03.10 -64 51 48.6           ~ 1540 0
4 NGC 3201 GlC 10 17 36.82 -46 24 44.9           ~ 1001 0
5 Cl Ruprecht 106 GlC 12 38 40.20 -51 09 01.0           ~ 413 0
6 NGC 5139 GlC 13 26 47.28 -47 28 46.1           ~ 3677 0
7 M 3 GlC 13 42 11.62 +28 22 38.2     6.39     ~ 2593 0
8 NGC 5286 GlC 13 46 26.81 -51 22 27.3           ~ 485 0
9 M 4 GlC 16 23 35.22 -26 31 32.7           ~ 1978 0
10 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
11 M 62 GlC 17 01 12.60 -30 06 44.5           ~ 668 0
12 M 19 GlC 17 02 37.69 -26 16 04.6   8.45 5.57     ~ 406 1
13 NGC 6362 GlC 17 31 54.99 -67 02 54.0           ~ 637 0
14 Cl Terzan 5 Cl* 17 48 05.00 -24 46 48.0           ~ 948 1
15 M 22 GlC 18 36 23.94 -23 54 17.1           ~ 1459 0
16 M 54 GlC 18 55 03.33 -30 28 47.5           ~ 1164 0
17 NAME SDG G 18 55 19.0 -30 32 43   4.5 3.6     ~ 2438 2
18 NGC 6752 GlC 19 10 52.11 -59 59 04.4           ~ 2121 0
19 Cl Terzan 7 GlC 19 17 43.92 -34 39 27.8           ~ 460 0
20 Cl Terzan 8 GlC 19 41 44.41 -33 59 58.1     11.54     ~ 357 0
21 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3274 0
22 M 2 GlC 21 33 27.02 -00 49 23.7     6.25     ~ 1114 1
23 Cl Pal 12 GlC 21 46 38.84 -21 15 09.4     11.89     ~ 548 0

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