NGC 5606
(fsr 1681; MWSC 2218)
0.95
UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
4.5 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 5606 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 moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (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.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 216.945 | -59.632 | 0.398 | -4.921 | -2.877 | -41.412 |
| Li et al. | 2025 | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | β |
| Almeida et al. | 2025 | 216.952 | -59.633 | β | β | β | β |
| Hunt & Reffert | 2024 | 216.956 | -59.63 | 0.389 | -4.992 | -2.892 | -54.014 |
| Celli et al. | 2024 | 216.946 | -59.632 | β | β | β | β |
| Cavallo et al. | 2024 | 216.959 | -59.633 | 0.392 | β | β | β |
| Hunt & Reffert | 2023 | 216.956 | -59.63 | 0.389 | -4.992 | -2.892 | -54.014 |
| Just et al. | 2023 | 216.933 | -59.628 | β | β | β | β |
| Jaehnig et al. | 2021 | 216.938 | -59.635 | 0.412 | -4.869 | -2.874 | β |
| Rain et al. | 2021 | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | β |
| Dias et al. | 2021 | 216.952 | -59.633 | 0.381 | -4.881 | -2.897 | β |
| Cantat-Gaudin et al. | 2020 | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | β |
| SΓ‘nchez et al. | 2020 | 216.946 | -59.632 | β | -4.886 | -3.209 | β |
| Cantat-Gaudin & Anders | 2020 | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | β |
| Bica et al. | 2019 | 217.174 | -59.763 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | β |
| Loktin & Popova | 2017 | 216.945 | -59.632 | β | -2.973 | -5.844 | -38.3 |
| Kharchenko et al. | 2016 | 216.933 | -59.628 | β | β | β | β |
| Dias et al. | 2014 | 216.946 | -59.632 | β | -3.5 | -5.11 | β |
| Kharchenko et al. | 2013 | 216.945 | -59.63 | β | -2.9 | -2.83 | -38.3 |
| Gozha et al. | 2012 | 216.946 | -59.632 | β | β | β | β |
| Piskunov et al. | 2008 | 216.94 | -59.626 | β | β | β | β |
| Kharchenko et al. | 2007 | 216.94 | -59.63 | β | 0.2 | β | -38.33 |
| Froebrich et al. | 2007 | 217.167 | -59.759 | β | β | β | β |
| van den Bergh | 2006 | 216.946 | -59.64 | β | β | β | β |
| Kharchenko et al. | 2005 | 216.94 | -59.63 | β | -4.78 | -3.26 | -38.33 |
| Kharchenko et al. | 2003 | 216.94 | -59.63 | β | -1.55 | -0.03 | β |
| Chen et al. | 2003 | 217.05 | -59.604 | β | -5.19 | -4.6 | -37.1 |
| Dias et al. | 2002 | 216.946 | -59.632 | β | -5.19 | -4.6 | -37.75 |
| Dambis | 1999 | 216.946 | -59.64 | 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 | 2.11 | 1.67 | β | 9 | -0.071 | β | β | β |
| Almeida et al. | 2025 | 2.34 | 1.70 | β | 10 | β | 310 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1104* | β | β |
| Celli et al. | 2024 | β | β | β | 18 | β | 308 | β | β |
| Cavallo et al. | 2024 | 1.85 | 1.64 | β | 10 | -0.160 | β | β | β |
| Hunt & Reffert | 2023 | 2.30 | 1.75 | 1.67 | 12 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 22 | β | 263 | β | β |
| Jaehnig et al. | 2021 | 2.42* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.48 | 1.46 | β | 12 | β | β | β | 0 |
| Dias et al. | 2021 | 2.34 | 1.70 | β | 10 | 0.143 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.49 | 1.69 | β | 18 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.48 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.48 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.80 | 1.46 | β | 12 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.14 | 1.42 | β | 22 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.14 | 1.42 | β | 22 | β | β | β | β |
| Gozha et al. | 2012 | 1.80 | β | β | 12 | 0.090 | 4266 | β | β |
| Piskunov et al. | 2008 | 1.80 | 1.46 | β | 7 | β | β | β | β |
| van den Bergh | 2006 | 1.80 | 1.46 | β | 12 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.80 | 1.46 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.80 | 1.40 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.80 | β | β | 10 | β | β | β | β |
| Dias et al. | 2002 | 1.80 | 1.47 | β | 12 | β | β | β | β |
| Dambis | 1999 | 1.80 | 1.53 | β | 10 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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