Collinder 440
(NGC 7128; MWSC 3554; OCL 218; FSR 0327)
0.97
UTI
0.83
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
95.2 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 440 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 325.992 | 53.715 | 0.268 | -4.065 | -4.131 | -53.53 |
| Almeida et al. | 2025 | 325.991 | 53.714 | β | β | β | β |
| Zhang et al. | 2024 | 325.989 | 53.716 | β | β | β | β |
| Hunt & Reffert | 2024 | 325.989 | 53.716 | 0.277 | -4.054 | -4.131 | -53.532 |
| Celli et al. | 2024 | 325.991 | 53.715 | β | β | β | β |
| Cavallo et al. | 2024 | 325.996 | 53.714 | 0.269 | β | β | β |
| Hunt & Reffert | 2023 | 325.989 | 53.716 | 0.277 | -4.054 | -4.131 | -53.532 |
| Almeida et al. | 2023 | 325.991 | 53.712 | β | β | β | β |
| Just et al. | 2023 | 325.955 | 53.722 | β | β | β | β |
| Jaehnig et al. | 2021 | 325.99 | 53.717 | 0.285 | -4.028 | -4.1 | β |
| Rain et al. | 2021 | 325.991 | 53.715 | 0.261 | -4.026 | -4.111 | β |
| Dias et al. | 2021 | 325.991 | 53.714 | 0.255 | -4.015 | -4.124 | β |
| Cantat-Gaudin et al. | 2020 | 325.991 | 53.715 | 0.261 | -4.026 | -4.111 | β |
| SΓ‘nchez et al. | 2020 | 325.988 | 53.715 | β | -3.925 | -4.245 | β |
| Cantat-Gaudin & Anders | 2020 | 325.991 | 53.715 | 0.261 | -4.026 | -4.111 | β |
| Dias et al. | 2019 | 325.992 | 53.715 | 0.261 | -4.026 | -4.111 | -54.93 |
| Bica et al. | 2019 | 325.995 | 53.706 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 325.991 | 53.715 | 0.261 | -4.026 | -4.111 | β |
| Loktin & Popova | 2017 | 325.995 | 53.715 | β | -5.17 | -4.84 | -48.2 |
| Kharchenko et al. | 2016 | 325.955 | 53.722 | β | β | β | β |
| Dias et al. | 2014 | 325.987 | 53.715 | β | -5.17 | -4.84 | β |
| Kharchenko et al. | 2013 | 325.96 | 53.725 | β | -6.9 | -2.76 | -48.2 |
| Gozha et al. | 2012 | 325.987 | 53.715 | β | β | β | β |
| Kharchenko et al. | 2012 | 325.96 | 53.725 | β | -6.9 | -2.76 | -48.25 |
| Kharchenko et al. | 2007 | 325.99 | 53.72 | β | 0.03 | β | β |
| van den Bergh | 2006 | 326.0 | 53.717 | β | β | β | β |
| Dias et al. | 2002 | 325.988 | 53.715 | β | -5.17 | -4.84 | -48.0 |
| Dambis | 1999 | 325.987 | 53.715 | 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 | 3.19 | 3.14 | 2.21 | 18 | -0.032 | 1236 | 0.6 | 0.0 |
| Almeida et al. | 2025 | 3.24 | 2.88 | β | 13 | β | 1053 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.320(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2643(1) | β | β |
| Celli et al. | 2024 | β | β | β | 26 | β | 1236 | β | β |
| Cavallo et al. | 2024 | 3.19 | 3.13 | β | 16 | 0.220 | β | β | β |
| Hunt & Reffert | 2023 | 3.33 | 3.19 | 2.21 | 18 | β | β | β | β |
| Almeida et al. | 2023 | 3.13 | 2.94 | β | 15 | -0.046 | 1366(1) | 0.60 | β |
| Just et al. | 2023 | β | β | β | 18 | β | 65 | β | β |
| Jaehnig et al. | 2021 | 3.48(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 3.45 | 3.13 | β | 18 | β | β | β | 0 |
| Dias et al. | 2021 | 3.24 | 2.88 | β | 13 | -0.032 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.21 | 2.59 | β | 26 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.45 | β | β | β | β | β | β | β |
| Dias et al. | 2019 | 4.82 | 2.85 | β | 14 | 0.223 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.45 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.31 | 3.14 | β | 19 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.30 | 3.41 | β | 18 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.30 | 3.41 | β | 18 | β | β | β | β |
| Gozha et al. | 2012 | 2.31 | β | β | 18 | β | β | β | β |
| Kharchenko et al. | 2012 | 2.30 | 3.41 | β | 18 | β | β | β | β |
| van den Bergh | 2006 | 2.31 | 3.16 | β | 18 | β | β | β | β |
| Dias et al. | 2002 | 2.31 | 3.16 | β | 18 | β | β | β | β |
| Dambis | 1999 | 2.01 | 5.08 | β | 25 | 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: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.