NGC 6531
(Melotte 188; Collinder 363; MWSC 2796; M 21; OCL 26; ESO 521 19)
0.96
UTI
0.79
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
70.1 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6531 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and mass parameters (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 271.046 | -22.503 | 0.799 | 0.542 | -1.45 | -4.885 |
| Almeida et al. | 2025 | 271.031 | -22.515 | β | β | β | β |
| Hunt & Reffert | 2024 | 271.042 | -22.5 | 0.801 | 0.538 | -1.464 | -5.191 |
| Celli et al. | 2024 | 271.036 | -22.505 | β | β | β | β |
| Cavallo et al. | 2024 | 271.041 | -22.523 | 0.798 | β | β | β |
| Hunt & Reffert | 2023 | 271.042 | -22.5 | 0.801 | 0.538 | -1.464 | -5.191 |
| Just et al. | 2023 | 271.042 | -22.491 | β | β | β | β |
| He et al. | 2022 | 271.036 | -22.511 | 0.807 | 0.535 | -1.476 | β |
| Jaehnig et al. | 2021 | 271.05 | -22.495 | 0.841 | 0.472 | -1.397 | β |
| Rain et al. | 2021 | 271.036 | -22.505 | 0.798 | 0.525 | -1.521 | β |
| Richer et al. | 2021 | 271.047 | -22.507 | 0.81 | 0.394 | -1.361 | β |
| Dias et al. | 2021 | 271.031 | -22.515 | 0.797 | 0.537 | -1.536 | β |
| Spina et al. | 2021 | 271.034 | -22.504 | 0.802 | 0.532 | -1.422 | β |
| Cantat-Gaudin et al. | 2020 | 271.036 | -22.505 | 0.798 | 0.525 | -1.521 | β |
| SΓ‘nchez et al. | 2020 | 271.054 | -22.49 | β | 0.597 | -1.404 | β |
| Cantat-Gaudin & Anders | 2020 | 271.036 | -22.505 | 0.798 | 0.525 | -1.521 | β |
| Bossini et al. | 2019 | 271.036 | -22.505 | β | β | β | β |
| Bica et al. | 2019 | 271.046 | -22.494 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 271.036 | -22.505 | 0.798 | 0.525 | -1.521 | β |
| Loktin & Popova | 2017 | 271.05 | -22.491 | β | 2.794 | -2.952 | -14.7 |
| Kharchenko et al. | 2016 | 271.042 | -22.491 | β | β | β | β |
| Dias et al. | 2014 | 271.054 | -22.49 | β | 0.55 | 0.15 | β |
| Kharchenko et al. | 2013 | 271.05 | -22.49 | β | 2.43 | -1.44 | -14.7 |
| Morales et al. | 2013 | 271.054 | -22.49 | β | β | β | β |
| Gozha et al. | 2012 | 271.054 | -22.49 | β | β | β | β |
| Bukowiecki et al. | 2011 | 271.012 | -22.493 | β | β | β | β |
| Piskunov et al. | 2008 | 271.046 | -22.494 | β | β | β | β |
| Kharchenko et al. | 2007 | 271.05 | -22.49 | β | 0.3 | β | -14.71 |
| Piskunov et al. | 2007 | 271.046 | -22.494 | β | β | β | β |
| Ahumada & Lapasset | 2007 | 271.05 | -22.483 | β | β | β | β |
| van den Bergh | 2006 | 271.05 | -22.483 | β | β | β | β |
| Kharchenko et al. | 2005 | 271.05 | -22.49 | β | 0.26 | -2.66 | -14.71 |
| Kharchenko et al. | 2003 | 271.05 | -22.49 | β | -0.38 | -2.47 | β |
| Chen et al. | 2003 | 271.109 | -22.492 | β | 2.28 | -3.05 | -16.0 |
| Dias et al. | 2002 | 271.054 | -22.49 | β | 2.28 | -3.05 | -13.49 |
| Dambis | 1999 | 271.054 | -22.49 | β | β | β | β |
| Lynga | 1987 | 271.157 | -22.495 | β | β | β | -12.0 |
| Sulentic et al. | 1973 | 271.153 | -22.498 | β | β | β | β |
π‘ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 1.21 | 0.88 | 1.3 | 11 | 0.000 | 668 | β | 0 |
| Liu et al. | 2025 | 1.49 | 0.28 | β | 11 | β | β | β | β |
| Almeida et al. | 2025 | 1.16 | 0.99 | β | 13 | β | 446 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 913(1) | β | β |
| Celli et al. | 2024 | β | β | β | 13 | β | 670 | β | β |
| Cavallo et al. | 2024 | 1.08 | 0.98 | β | 9 | -0.130 | β | β | β |
| Hunt & Reffert | 2023 | 1.19 | 0.80 | 1.30 | 5 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 7 | β | 117 | β | β |
| He et al. | 2022 | β | 1.10 | β | 6 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.19(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.21 | 0.76 | β | 11 | β | β | β | 0 |
| Richer et al. | 2021 | β | 1.61 | β | 12 | β | β | β | β |
| Dias et al. | 2021 | 1.16 | 0.99 | β | 13 | 0.090 | β | β | β |
| Spina et al. | 2021 | 1.25 | β | β | 13 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.16 | 0.67 | β | 13 | β | β | β | β |
| Kounkel et al. | 2020 | 1.19 | 1.13 | β | 11 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.21 | β | β | β | β | β | β | β |
| Bossini et al. | 2019 | 1.09 | 0.76 | β | 11 | 0.000 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.21 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.21 | 0.89 | β | 12 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.19 | 1.09 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.19 | 1.09 | β | 7 | β | β | β | β |
| Morales et al. | 2013 | 1.21 | β | β | 12 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 667 | β | β |
| Gozha et al. | 2012 | 1.21 | β | β | 12 | β | 2512 | β | β |
| Bukowiecki et al. | 2011 | 0.80(1) | 0.76 | β | 16 | β | β | β | β |
| Piskunov et al. | 2008 | 1.21 | 0.88 | β | 7 | β | 783(1) | β | β |
| Piskunov et al. | 2007 | 1.21 | 0.88 | β | 7 | β | 170 | β | β |
| Ahumada & Lapasset | 2007 | β | 0.88 | β | 12 | β | β | β | 0 |
| van den Bergh | 2006 | 1.21 | 0.88 | β | 12 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.21 | 0.88 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.21 | 0.79 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.21 | β | β | 10 | β | β | β | β |
| Dias et al. | 2002 | 1.21 | 0.89 | β | 12 | β | β | β | β |
| Dambis | 1999 | 1.03 | 0.88 | β | 4 | β | β | β | β |
| Lynga | 1987 | 1.30 | 0.91 | β | 5 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 129 along with Collinder_367.
Palma et al. (2025)
Classified as genetic pair P216, along with HSC_106.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 1.00 (50th percentile), true positive (human-assigned).
Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=7.873, Av=0.636, [Fe/H]=0.00 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108).
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.