IC 4725
(Melotte 204; Collinder 382; MWSC 2940; M 25; OCL 38; ESO 591 06; FoF 2292)
0.98
UTI
0.9
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
58.5 [N/pc2]
- CN 0.9 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
IC 4725 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate 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 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 | 277.938 | -19.117 | 1.512 | -1.687 | -6.143 | 2.392 |
| Li et al. | 2025 | 277.937 | -19.114 | 1.514 | -1.688 | -6.117 | â |
| Wei et al. | 2025 | 277.955 | -19.122 | 1.513 | -1.686 | -6.163 | â |
| Almeida et al. | 2025 | 277.938 | -19.112 | â | â | â | â |
| Alfonso et al. | 2024 | 277.944 | -19.119 | 1.475 | -1.686 | -6.156 | â |
| Hunt & Reffert | 2024 | 277.942 | -19.131 | 1.512 | -1.692 | -6.165 | 2.015 |
| Cavallo et al. | 2024 | 277.949 | -19.122 | 1.512 | â | â | â |
| Hunt & Reffert | 2023 | 277.942 | -19.131 | 1.512 | -1.692 | -6.165 | 2.015 |
| Cordoni et al. | 2023 | 277.938 | -19.112 | 1.513 | -1.687 | -6.112 | â |
| Just et al. | 2023 | 277.92 | -19.111 | â | â | â | â |
| He et al. | 2022 | 277.947 | -19.127 | 1.515 | -1.687 | -6.15 | â |
| Tarricq et al. | 2022 | 277.93 | -19.125 | 1.513 | -1.694 | -6.141 | â |
| Jaehnig et al. | 2021 | 277.962 | -19.101 | 1.541 | -1.663 | -6.102 | â |
| Rain et al. | 2021 | 277.937 | -19.114 | 1.514 | -1.688 | -6.117 | â |
| Dias et al. | 2021 | 277.938 | -19.112 | 1.513 | -1.687 | -6.112 | 10.314 |
| Spina et al. | 2021 | 277.938 | -19.112 | 1.51 | -1.681 | -6.113 | â |
| Cantat-Gaudin et al. | 2020 | 277.937 | -19.114 | 1.514 | -1.688 | -6.117 | â |
| Cantat-Gaudin & Anders | 2020 | 277.937 | -19.114 | 1.514 | -1.688 | -6.117 | â |
| Liu & Pang | 2019 | 277.954 | -19.103 | 1.511 | -1.696 | -6.124 | â |
| Bossini et al. | 2019 | 277.937 | -19.114 | â | â | â | â |
| Soubiran et al. | 2018 | 277.937 | -19.114 | â | â | â | 3.09 |
| Bica et al. | 2019 | 277.936 | -19.126 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 277.937 | -19.114 | 1.514 | -1.688 | -6.117 | â |
| Loktin & Popova | 2017 | 277.95 | -19.118 | â | -4.01 | -5.7 | -1.8 |
| Kharchenko et al. | 2016 | 277.92 | -19.111 | â | â | â | â |
| Dias et al. | 2014 | 277.946 | -19.117 | â | -2.54 | -3.99 | â |
| Kharchenko et al. | 2013 | 277.927 | -19.11 | â | -2.2 | -6.09 | -1.8 |
| Gozha et al. | 2012 | 277.946 | -19.117 | â | â | â | â |
| Piskunov et al. | 2008 | 277.913 | -19.126 | â | â | â | â |
| Kharchenko et al. | 2007 | 277.95 | -19.12 | â | 0.6 | â | -1.81 |
| Piskunov et al. | 2007 | 277.913 | -19.126 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 277.95 | -19.117 | â | â | â | â |
| van den Bergh | 2006 | 277.925 | -19.117 | â | â | â | â |
| Kharchenko et al. | 2005 | 277.92 | -19.12 | â | -2.73 | -4.95 | -1.81 |
| Kharchenko et al. | 2003 | 277.86 | -19.16 | â | -3.37 | -5.73 | â |
| Chen et al. | 2003 | 277.95 | -19.177 | â | -2.78 | -6.15 | 3.0 |
| Dias et al. | 2002 | 277.946 | -19.117 | â | -4.01 | -5.7 | 2.4 |
| Dambis | 1999 | 277.946 | -19.117 | â | â | â | â |
| Lynga | 1987 | 277.93 | -19.246 | â | â | â | 3.0 |
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 | 0.64 | 1.42 | 1.57 | 93 | 0.169 | 1261 | 0.355 | 0 |
| Li et al. | 2025 | 0.59 | 1.25 | â | 116 | -0.054 | â | â | â |
| Wei et al. | 2025 | 1.10 | 1.64 | â | 66 | 0.000 | 1694 | 0.46 | â |
| Almeida et al. | 2025 | 0.64 | 1.36 | â | 167 | â | 1254 | â | â |
| Alfonso et al. | 2024 | 0.70 | 0.84 | â | 462 | 0.172 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2248(1) | â | â |
| Cavallo et al. | 2024 | 0.65 | 1.36 | â | 170 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 0.62 | 1.36 | 1.57 | 96 | â | â | â | â |
| Cordoni et al. | 2023 | 0.64 | 1.36 | â | 167 | 0.169 | 1268 | 0.25 | 0(1) |
| Just et al. | 2023 | â | â | â | 93 | â | 57 | â | â |
| He et al. | 2022 | â | 1.65 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.69 | â | â | 112 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.65(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.65 | 1.10 | â | 95 | â | â | â | 0 |
| Dias et al. | 2021 | 0.64 | 1.36 | â | 167 | 0.169 | â | â | â |
| Spina et al. | 2021 | 0.66 | â | â | 112 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.70 | 0.84 | â | 112 | â | â | â | â |
| Kounkel et al. | 2020 | 0.65 | 1.13 | â | 162 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.65 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 68 | -0.250 | â | â | â |
| Bossini et al. | 2019 | 0.68 | 1.09 | â | 96 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.65 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.62 | 1.49 | â | 92 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.56 | 1.51 | â | 93 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.56 | 1.51 | â | 93 | -0.257 | â | â | â |
| Gozha et al. | 2012 | 0.62 | â | â | 92 | 0.170 | 1096 | â | â |
| Piskunov et al. | 2008 | 0.62 | 1.42 | â | 68 | â | 1486(1) | â | â |
| Piskunov et al. | 2007 | 0.62 | 1.42 | â | 68 | â | 475 | â | â |
| Ahumada & Lapasset | 2007 | â | 1.51 | â | 93 | â | â | â | 5 |
| van den Bergh | 2006 | 0.62 | 1.51 | â | 91 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.62 | 1.42 | â | 68 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.62 | 1.48 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.62 | 1.50 | â | 90 | 0.170(1) | â | â | â |
| Dias et al. | 2002 | 0.62 | 1.50 | â | 92 | 0.170 | â | â | â |
| Dambis | 1999 | 0.53 | 1.53 | â | 40 | â | â | â | â |
| Lynga | 1987 | 0.56 | 1.51 | â | 89 | -0.060 | 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: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
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)=7.984, Av=7.984, [Fe/H]=0.00 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108). Ahumada & Lapasset (2007A&A...463..789A, Cat. J/A+A/463/789) cite stars DR2 4092873695966184320=HD 170475, DR2 4092906509511384064=HD 170682, DR2 4092908360541000320= HD 170719, DR2 4092856790967940608=HD 170835, DR2 4092855416578333952= HD 170836 as possible blue stragglers. HD 170682 and HD 170719 are not members according to Cantat-Gaudin et al. (2018A&A...618A..93C, Cat. J/A+A18/A93). HD 170475, HD 170835, HD 170836 are members but located in the turnoff.
Ahumada & Lapasset (2007)
Spectra: Star 1=HD 170475, B8III/IV (1975MSS...C01....0H); star 50=HD 170682, B6V (1957MNRAS.117..193F); star 91=HD 170719, B9V (1957MNRAS.117..193F); star 163=HD 170835, B2.5Vne (1977ApJS...35..111G); star 167=HD 170836, B8II (1975MSS...C01....0H).