NGC 4609
(MWSC 2062; FoF 1129)
0.92
UTI
0.86
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
5.9 [arcmin]
- CN 0.86 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 4609 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 190.574 | -62.994 | 0.678 | -4.9 | -1.007 | 3.553 |
| Li et al. | 2025 | 190.582 | -62.995 | 0.66 | -4.87 | -1.045 | β |
| Wei et al. | 2025 | 190.537 | -62.989 | 0.679 | -4.887 | -0.985 | β |
| Almeida et al. | 2025 | 190.583 | -62.983 | β | β | β | β |
| Hunt & Reffert | 2024 | 190.567 | -62.993 | 0.688 | -4.892 | -1.002 | -4.072 |
| Cavallo et al. | 2024 | 190.561 | -62.981 | 0.687 | β | β | β |
| Hunt & Reffert | 2023 | 190.567 | -62.993 | 0.688 | -4.892 | -1.002 | -4.072 |
| Almeida et al. | 2023 | 190.632 | -62.993 | β | β | β | β |
| Cordoni et al. | 2023 | 190.583 | -62.983 | 0.669 | -4.876 | -1.029 | β |
| Just et al. | 2023 | 190.565 | -62.987 | β | β | β | β |
| Tarricq et al. | 2022 | 190.538 | -62.99 | 0.69 | -4.894 | -1.009 | β |
| Jaehnig et al. | 2021 | 190.563 | -62.997 | 0.692 | -4.868 | -1.05 | β |
| Rain et al. | 2021 | 190.582 | -62.995 | 0.66 | -4.87 | -1.045 | β |
| Dias et al. | 2021 | 190.583 | -62.983 | 0.669 | -4.876 | -1.029 | β |
| Cantat-Gaudin et al. | 2020 | 190.582 | -62.995 | 0.66 | -4.87 | -1.045 | β |
| SΓ‘nchez et al. | 2020 | 190.575 | -62.995 | β | -4.879 | -1.059 | β |
| Cantat-Gaudin & Anders | 2020 | 190.582 | -62.995 | 0.66 | -4.87 | -1.045 | β |
| Liu & Pang | 2019 | 190.589 | -62.991 | 0.676 | -4.877 | -1.028 | β |
| Bossini et al. | 2019 | 190.582 | -62.995 | β | β | β | β |
| Soubiran et al. | 2018 | 190.582 | -62.995 | β | β | β | -25.22 |
| Cantat-Gaudin et al. | 2018 | 190.582 | -62.995 | 0.66 | -4.87 | -1.045 | β |
| Loktin & Popova | 2017 | 190.575 | -62.995 | β | -8.164 | -1.542 | 22.0 |
| Kharchenko et al. | 2016 | 190.565 | -62.987 | β | β | β | β |
| Dias et al. | 2014 | 190.575 | -62.995 | β | -3.83 | -1.56 | β |
| Kharchenko et al. | 2013 | 190.575 | -62.99 | β | -7.57 | -1.36 | 22.0 |
| Gozha et al. | 2012 | 190.575 | -62.995 | β | β | β | β |
| Piskunov et al. | 2008 | 190.565 | -62.983 | β | β | β | β |
| Kharchenko et al. | 2007 | 190.57 | -62.99 | β | 0.14 | β | 22.0 |
| van den Bergh | 2006 | 190.575 | -62.983 | β | β | β | β |
| Kharchenko et al. | 2005 | 190.57 | -62.99 | β | -8.92 | -1.67 | β |
| Kharchenko et al. | 2003 | 190.56 | -62.99 | β | -9.21 | -2.69 | β |
| Dias et al. | 2002 | 190.575 | -62.995 | β | -9.45 | -6.52 | -21.3 |
| Dambis | 1999 | 190.575 | -62.995 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.31 | 1.12 | β | 59 | -0.046 | β | β | β |
| Wei et al. | 2025 | 2.23 | 1.29 | β | 178 | 0.250 | 960 | 0.42 | β |
| Almeida et al. | 2025 | 1.37 | 1.23 | β | 53 | β | 1055 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1514* | β | β |
| Cavallo et al. | 2024 | 1.29 | 1.22 | β | 107 | -0.050 | β | β | β |
| Hunt & Reffert | 2023 | 1.38 | 1.04 | 0.91 | 66 | β | β | β | β |
| Almeida et al. | 2023 | 1.37 | 1.23 | β | 76 | 0.097 | 943* | 0.58 | β |
| Cordoni et al. | 2023 | 1.37 | 1.23 | β | 53 | 0.023 | 4890 | 0.46 | 0.00 |
| Just et al. | 2023 | β | β | β | 126 | β | 119 | β | β |
| Tarricq et al. | 2022 | 1.38 | β | β | 83 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.44* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.45 | 1.05 | β | 33 | β | β | β | 0 |
| Dias et al. | 2021 | 1.37 | 1.23 | β | 53 | 0.023 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.42 | 0.88 | β | 81 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.45 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 35 | -0.250 | β | β | β |
| Bossini et al. | 2019 | 1.50 | 1.07 | β | 33 | 0.050 | β | β | β |
| Soubiran et al. | 2018 | 1.45 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.45 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.24 | 1.02 | β | 79 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.31 | 1.13 | β | 126 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.31 | 1.13 | β | 126 | β | β | β | β |
| Gozha et al. | 2012 | 1.22 | β | β | 50 | 0.050 | 87 | β | β |
| Piskunov et al. | 2008 | 1.22 | 1.02 | β | 60 | β | β | β | β |
| van den Bergh | 2006 | 1.22 | 1.02 | β | 78 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.22 | 1.02 | β | 60 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.22 | 1.02 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.32 | 1.15 | β | 50 | 0.050 | β | β | β |
| Dambis | 1999 | 1.23 | 1.11 | β | 32 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.