Melotte 109
(Collinder 252; VDBH 127; NGC 4103; MWSC 1997; OCL 871; vdBergh-Hagen 127; ESO 130 05; FoF 420)
0.96
UTI
0.82
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
60.0 [N/pc2]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Melotte 109 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 181.65 | -61.244 | 0.488 | -6.198 | 0.154 | -24.485 |
| Wei et al. | 2025 | 181.612 | -61.239 | 0.502 | -6.186 | 0.173 | β |
| Almeida et al. | 2025 | 181.603 | -61.249 | β | β | β | β |
| Hunt & Reffert | 2024 | 181.656 | -61.247 | 0.493 | -6.207 | 0.185 | -33.543 |
| Celli et al. | 2024 | 181.628 | -61.245 | β | β | β | β |
| Cavallo et al. | 2024 | 181.642 | -61.244 | 0.494 | β | β | β |
| Hunt & Reffert | 2023 | 181.656 | -61.247 | 0.493 | -6.207 | 0.185 | -33.543 |
| Just et al. | 2023 | 181.656 | -61.246 | β | β | β | β |
| Jaehnig et al. | 2021 | 181.639 | -61.243 | 0.495 | -6.209 | 0.144 | β |
| Rain et al. | 2021 | 181.628 | -61.245 | 0.473 | -6.184 | 0.075 | β |
| Dias et al. | 2021 | 181.603 | -61.249 | 0.473 | -6.19 | 0.088 | -24.863 |
| Cantat-Gaudin et al. | 2020 | 181.628 | -61.245 | 0.473 | -6.184 | 0.075 | β |
| SΓ‘nchez et al. | 2020 | 181.667 | -61.25 | β | -6.141 | 0.115 | β |
| Cantat-Gaudin & Anders | 2020 | 181.628 | -61.245 | 0.473 | -6.184 | 0.075 | β |
| Liu & Pang | 2019 | 181.634 | -61.249 | 0.473 | -6.215 | 0.15 | β |
| Bossini et al. | 2019 | 181.628 | -61.245 | β | β | β | β |
| Bica et al. | 2019 | 181.657 | -61.254 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 181.628 | -61.245 | 0.473 | -6.184 | 0.075 | β |
| Loktin & Popova | 2017 | 181.665 | -61.25 | β | -3.568 | 1.282 | -12.0 |
| Kharchenko et al. | 2016 | 181.656 | -61.246 | β | β | β | β |
| Dias et al. | 2014 | 181.667 | -61.25 | β | -4.57 | 0.18 | β |
| Kharchenko et al. | 2013 | 181.665 | -61.25 | β | -5.42 | 0.98 | -12.0 |
| Gozha et al. | 2012 | 181.667 | -61.25 | β | β | β | β |
| Piskunov et al. | 2008 | 181.661 | -61.245 | β | β | β | β |
| Kharchenko et al. | 2007 | 181.66 | -61.25 | β | 0.23 | β | -12.0 |
| van den Bergh | 2006 | 181.678 | -61.256 | β | β | β | β |
| Kharchenko et al. | 2005 | 181.66 | -61.25 | β | -5.04 | -0.95 | -12.0 |
| Kharchenko et al. | 2003 | 181.68 | -61.25 | β | -5.01 | -0.91 | β |
| Dias et al. | 2002 | 181.667 | -61.25 | β | -7.3 | -0.13 | -12.0 |
| Dambis | 1999 | 181.678 | -61.256 | 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 | 1.83 | 0.91 | 1.17 | 29 | 0.010 | 1400 | 0.39 | 0.0 |
| Wei et al. | 2025 | 2.59 | 1.43 | β | 26 | -0.500 | 1564 | 0.39 | β |
| Almeida et al. | 2025 | 1.87 | 1.10 | β | 29 | β | 1316 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2143(1) | β | β |
| Celli et al. | 2024 | β | β | β | 21 | β | 1483 | β | β |
| Cavallo et al. | 2024 | 1.83 | 1.04 | β | 31 | 0.020 | β | β | β |
| Hunt & Reffert | 2023 | 1.89 | 0.90 | 1.17 | 30 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 57 | β | 366 | β | β |
| Jaehnig et al. | 2021 | 2.03(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.99 | 0.90 | β | 27 | β | β | β | 0 |
| Dias et al. | 2021 | 1.87 | 1.10 | β | 29 | 0.128 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.06 | 0.85 | β | 21 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.99 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 83 | 0.500 | β | β | β |
| Bossini et al. | 2019 | 1.92 | 0.99 | β | 27 | 0.000 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.99 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.67 | 0.85 | β | 29 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.66 | 0.94 | β | 57 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.66 | 0.94 | β | 57 | β | β | β | β |
| Gozha et al. | 2012 | 1.63 | β | β | 25 | -0.470 | 1175 | β | β |
| Piskunov et al. | 2008 | 1.66 | 0.87 | β | 39 | β | β | β | β |
| van den Bergh | 2006 | 1.63 | 0.90 | β | 25 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.66 | 0.87 | β | 39 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.63 | 0.90 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.63 | 0.91 | β | 25 | β | β | β | β |
| Dambis | 1999 | 1.77 | 0.96 | 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: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.