NGC 6756
(Collinder 398; MWSC 3052; OCL 99; FSR 0113)
0.91
UTI
0.87
CN
1.0
Cdens
1.0
CC3
0.83
Clit
1.0
Cdup
Stellar density (N50/rad)
145.8 [N/pc2]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.83 Well-studied
- Cdup 1.0 Unique
Overview
NGC 6756 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is 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 | 287.181 | 4.71 | 0.307 | -1.55 | -3.662 | 48.759 |
| Otto et al. | 2026 | 287.181 | 4.711 | β | -1.58 | -3.63 | 47.1 |
| Li et al. | 2025 | 287.181 | 4.711 | 0.281 | -1.584 | -3.631 | β |
| Almeida et al. | 2025 | 287.184 | 4.711 | β | β | β | β |
| Hunt & Reffert | 2024 | 287.181 | 4.711 | 0.312 | -1.546 | -3.665 | 55.282 |
| Cavallo et al. | 2024 | 287.182 | 4.709 | 0.308 | β | β | β |
| Hunt & Reffert | 2023 | 287.181 | 4.711 | 0.312 | -1.546 | -3.665 | 55.282 |
| Just et al. | 2023 | 287.18 | 4.715 | β | β | β | β |
| Dias et al. | 2021 | 287.184 | 4.711 | 0.283 | -1.586 | -3.628 | β |
| Cantat-Gaudin et al. | 2020 | 287.181 | 4.711 | 0.281 | -1.584 | -3.631 | β |
| SΓ‘nchez et al. | 2020 | 287.175 | 4.705 | β | -1.712 | -3.695 | β |
| Cantat-Gaudin & Anders | 2020 | 287.181 | 4.711 | 0.281 | -1.584 | -3.631 | β |
| Bica et al. | 2019 | 287.166 | 4.712 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 287.181 | 4.711 | 0.281 | -1.584 | -3.631 | β |
| Loktin & Popova | 2017 | 287.19 | 4.717 | β | -5.33 | -3.399 | β |
| Kharchenko et al. | 2016 | 287.18 | 4.715 | β | β | β | β |
| Dias et al. | 2014 | 287.175 | 4.705 | β | -1.03 | -3.43 | β |
| Kharchenko et al. | 2013 | 287.187 | 4.717 | β | -4.68 | -4.35 | β |
| Bukowiecki et al. | 2011 | 287.183 | 4.715 | β | β | β | β |
| van den Bergh | 2006 | 287.175 | 4.683 | β | β | β | β |
| Dias et al. | 2002 | 287.175 | 4.705 | β | -1.03 | -3.43 | β |
| Lynga | 1987 | 287.17 | 4.676 | β | β | β | β |
| Sulentic et al. | 1973 | 287.16 | 4.657 | 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 | 2.81 | 3.345 | 2.04 | 70 | 0.100 | 1978 | β | β |
| Otto et al. | 2026 | β | β | β | 48 | -0.060(15) | β | β | β |
| Li et al. | 2025 | 1.22 | 1.87 | β | 2667 | 0.049 | β | β | β |
| Almeida et al. | 2025 | 2.81 | 3.15 | β | 27 | β | 2380 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 4519(1) | β | β |
| Cavallo et al. | 2024 | 3.09 | 3.41 | β | 162 | 0.610 | β | β | β |
| Hunt & Reffert | 2023 | 2.89 | 3.55 | 2.04 | 47 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 251 | β | 219 | β | β |
| Dias et al. | 2021 | 2.81 | 3.15 | β | 27 | 0.324 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.16 | 3.17 | β | 48 | β | β | β | β |
| Kounkel et al. | 2020 | 2.97 | 3.28 | β | 288 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.22 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.22 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.21 | 2.39 | β | 646 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.95 | 3.42 | β | 251 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.95 | 3.42 | β | 251 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 1575 | β | β |
| Bukowiecki et al. | 2011 | 1.86(1) | 2.93 | β | 79 | β | β | β | β |
| van den Bergh | 2006 | 1.51 | 3.72 | β | 62 | β | β | β | β |
| Dias et al. | 2002 | 1.51 | 3.72 | β | 62 | 0.100 | β | β | β |
| Lynga | 1987 | 1.65 | 4.48 | β | 47 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg25' along with Czernik 39 and NGC 6755.