NGC 5606
(fsr 1681)
Summary
NGC 5606 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is very well-studied in the literature.
This object shares a small percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 216.946 | -59.64 | – | – | – | – |
| Dias et al. (2002) | 216.946 | -59.632 | – | -5.19 | -4.6 | -37.75 |
| Chen et al. (2003) | 217.05 | -59.604 | – | -5.19 | -4.6 | -37.1 |
| Froebrich et al. (2007) | 217.167 | -59.759 | – | – | – | – |
| Piskunov et al. (2008) | 216.94 | -59.626 | – | – | – | – |
| Kharchenko et al. (2012) | 216.945 | -59.63 | – | -2.9 | -2.83 | – |
| Loktin & Popova (2017) | 216.945 | -59.632 | – | -2.973 | -5.844 | -38.3 |
| Cantat-Gaudin et al. (2018) | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | – |
| Bica et al. (2019) | 217.174 | -59.763 | – | – | – | – |
| Cantat-Gaudin et al. (2020) | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | – |
| Dias et al. (2021) | 216.952 | -59.633 | 0.381 | -4.881 | -2.897 | – |
| Rain et al. (2021) | 216.946 | -59.632 | 0.374 | -4.88 | -2.897 | – |
| Jaehnig et al. (2021) | 216.938 | -59.635 | 0.412 | -4.869 | -2.874 | – |
| Hunt & Reffert (2023) | 216.956 | -59.63 | 0.389 | -4.992 | -2.892 | -54.014 |
| Cavallo et al. (2024) | 216.959 | -59.633 | 0.392 | – | – | – |
| Celli et al. (2024) | 216.946 | -59.632 | – | – | – | – |
| Hunt & Reffert (2024) | 216.956 | -59.63 | 0.389 | -4.992 | -2.892 | -54.014 |
| Almeida et al. (2025) | 216.952 | -59.633 | – | – | – | – |
| UCC | 216.945 | -59.632 | 0.398 | -4.921 | -2.877 | -41.412 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.495, DM0=11.28, log_age_=7.0 |
| Dias et al. (2002) | E(B-V)=0.474, Dist=1805.0, Age=7.075 |
| Chen et al. (2003) | HDis=1805, Age=0.01 |
| Piskunov et al. (2008) | E(B-V)=0.47, Dist=1805, logt=6.84, logMA=3.634 |
| Kharchenko et al. (2012) | e_bv=0.458, distance=2141, log_age=7.35 |
| Loktin & Popova (2017) | E(B-V)=0.471, Dist=1805, logt=7.084 |
| Cantat-Gaudin et al. (2018) | dmode=2480.0 |
| Cantat-Gaudin et al. (2020) | AVNN=1.69, DistPc=2493.0, AgeNN=7.26 |
| Dias et al. (2021) | Av=1.696, Dist=2344, logage=7.004, [Fe/H]=0.143 |
| Rain et al. (2021) | E(B-V)=0.47, Dist=2480.0, log(Age)=7.07, NBSS=0 |
| Jaehnig et al. (2021) | dmode=2.423 |
| Hunt & Reffert (2023) | AV50=1.754, diffAV50=1.669, MOD50=11.807, logAge50=7.083 |
| Cavallo et al. (2024) | AV50=1.64, dMod50=11.33, logAge50=7.01, [Fe/H]50=-0.16 |
| Celli et al. (2024) | Age=18.2, Mc=307.6 |
| Hunt & Reffert (2024) | MassJ=1103.61, MassTot=1166.29 |
| Almeida et al. (2025) | AV=1.696, Dist=2344, logAge=7.004, MassRk=310.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0612 | 23.1 | 216.95 | -59.63 | 0.41 | -4.88 | -2.89 | -119.27 | 0.0 |