NGC 4439
(MWSC 2035)
0.88
UTI
0.67
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
12.3 [N/pc2]
- CN 0.67 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 4439 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (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 | 99999â | 187.115 | -60.096 | 0.501 | -7.124 | -0.432 | -24.978 |
| Li et al. | 2025 | 187.119 | -60.097 | 0.474 | -7.089 | -0.413 | â |
| Almeida et al. | 2025 | 187.121 | -60.098 | â | â | â | â |
| Hunt & Reffert | 2024 | 187.111 | -60.097 | 0.499 | -7.175 | -0.434 | -19.882 |
| Cavallo et al. | 2024 | 187.102 | -60.092 | 0.501 | â | â | â |
| Hunt & Reffert | 2023 | 187.111 | -60.097 | 0.499 | -7.175 | -0.434 | -19.882 |
| Almeida et al. | 2023 | 187.121 | -60.102 | â | â | â | â |
| Just et al. | 2023 | 187.108 | -60.107 | â | â | â | â |
| Jaehnig et al. | 2021 | 187.105 | -60.109 | 0.512 | -7.116 | -0.461 | â |
| Rain et al. | 2021 | 187.119 | -60.097 | 0.474 | -7.089 | -0.413 | â |
| Dias et al. | 2021 | 187.121 | -60.098 | 0.473 | -7.054 | -0.374 | â |
| Cantat-Gaudin et al. | 2020 | 187.119 | -60.097 | 0.474 | -7.089 | -0.413 | â |
| Cantat-Gaudin & Anders | 2020 | 187.119 | -60.097 | 0.474 | -7.089 | -0.413 | â |
| Bossini et al. | 2019 | 187.119 | -60.097 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 187.119 | -60.097 | 0.474 | -7.089 | -0.413 | â |
| Dias et al. | 2018 | â | â | â | -7.57 | -0.98 | â |
| Dib et al. | 2018 | 187.117 | -60.11 | â | â | â | â |
| Loktin & Popova | 2017 | 187.11 | -60.105 | â | -12.942 | -5.335 | â |
| Sampedro et al. | 2017 | 187.113 | -60.105 | -4.99 | -2.59 | â | â |
| Joshi et al. | 2016 | 187.117 | -60.11 | â | â | â | â |
| Kharchenko et al. | 2016 | 187.108 | -60.107 | â | â | â | â |
| Dias et al. | 2014 | 187.112 | -60.105 | â | -4.92 | -2.78 | â |
| Kharchenko et al. | 2013 | 187.117 | -60.11 | â | -11.4 | -4.73 | â |
| Piskunov et al. | 2008 | 187.098 | -60.093 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 187.1 | -60.1 | â | â | â | â |
| van den Bergh | 2006 | 187.1 | -60.1 | â | â | â | â |
| Kharchenko et al. | 2005 | 187.11 | -60.1 | â | -10.8 | -5.04 | â |
| Kharchenko et al. | 2003 | 187.11 | -60.1 | â | -12.18 | -6.63 | â |
| Dias et al. | 2002 | 187.113 | -60.105 | â | -10.49 | -0.85 | â |
| Dambis | 1999 | 187.1 | -60.1 | â | â | â | â |
| Lynga | 1987 | 187.12 | -60.084 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 186.4 | -59.817 | â | â | â | â |
| Sulentic et al. | 1973 | 187.05 | -60.088 | â | â | â | â |
đĄ 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 | 99999â | 1.78 | 1.1 | 0.7 | 53 | 0.000 | 282 | 0.53 | 0 |
| Li et al. | 2025 | 1.67 | 1.14 | â | 58 | -0.049 | â | â | â |
| Almeida et al. | 2025 | 1.79 | 1.25 | â | 51 | â | 297 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 473(1) | â | â |
| Cavallo et al. | 2024 | 1.76 | 1.40 | â | 39 | -0.130 | â | â | â |
| Hunt & Reffert | 2023 | 1.82 | 0.97 | 0.70 | 94 | â | â | â | â |
| Almeida et al. | 2023 | 1.78 | 1.23 | â | 53 | 0.055 | 282(1) | 0.53 | â |
| Just et al. | 2023 | â | â | â | 51 | â | 203 | â | â |
| Jaehnig et al. | 2021 | 1.98(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.99 | 1.07 | â | 59 | â | â | â | 0 |
| Dias et al. | 2021 | 1.79 | 1.25 | â | 51 | 0.019 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.01 | 0.99 | â | 52 | â | â | â | â |
| Kounkel et al. | 2020 | 2.09 | 1.30 | â | 60 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.99 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 2.05 | 1.06 | â | 60 | 0.000 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.99 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.66 | â | â | 51 | â | â | â | â |
| Loktin & Popova | 2017 | 1.81 | 1.11 | â | 74 | â | â | â | â |
| Joshi et al. | 2016 | 1.66 | 0.98 | â | 51 | â | 19 | â | â |
| Kharchenko et al. | 2016 | 1.66 | 0.98 | â | 51 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.66 | 0.98 | â | 51 | â | â | â | â |
| Piskunov et al. | 2008 | 1.78 | 1.10 | â | 51 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 1.10 | â | 81 | â | â | â | 0 |
| van den Bergh | 2006 | 1.78 | 1.10 | â | 81 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.78 | 1.10 | â | 51 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.78 | 1.10 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.78 | 1.10 | â | 81 | â | â | â | â |
| Dambis | 1999 | 1.56 | 1.06 | â | 63 | â | â | â | â |
| Lynga | 1987 | 1.60 | 0.98 | â | 63 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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 class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=7.778, Av=1.064, [Fe/H]=0.00 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108). The distance d=1657.6 (dmode+01) of Cantat-Gaudin et al. (2018A&A...618A..93C, Cat. J/A+A18/A93) was use to fit the isochrone.
Ahumada & Lapasset (2007)
The apparent cluster diameter is from (1973A&AS...10..135M).