NGC 3590
(MWSC 1920; FoF 237)
Summary
NGC 3590 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is very well-studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 168.246 | -60.788 | – | – | – | – |
| Dias et al. (2002) | 168.246 | -60.788 | – | -3.3 | -1.28 | -7.33 |
| Kharchenko et al. (2003) | 168.25 | -60.78 | – | -5.35 | 1.74 | – |
| Kharchenko et al. (2005) | 168.25 | -60.78 | – | -6.51 | 1.48 | -7.33 |
| Kharchenko et al. (2007) | 168.24 | -60.79 | – | 0.17 | – | -7.33 |
| Piskunov et al. (2008) | 168.245 | -60.779 | – | – | – | – |
| Kharchenko et al. (2013) | 168.258 | -60.775 | – | -6.61 | 1.55 | -7.3 |
| Kharchenko et al. (2016) | 168.251 | -60.772 | – | – | – | – |
| Loktin & Popova (2017) | 168.24 | -60.788 | – | -3.3 | -1.28 | -7.3 |
| Cantat-Gaudin et al. (2018) | 168.262 | -60.79 | 0.361 | -6.1 | 1.013 | – |
| Soubiran et al. (2018) | 168.262 | -60.79 | – | – | – | 6.88 |
| Liu & Pang (2019) | 168.249 | -60.777 | 0.355 | -6.108 | 1.224 | – |
| Cantat-Gaudin et al. (2020) | 168.262 | -60.79 | 0.361 | -6.1 | 1.013 | – |
| Dias et al. (2021) | 168.262 | -60.788 | 0.362 | -6.116 | 1.023 | – |
| Rain et al. (2021) | 168.262 | -60.79 | 0.361 | -6.1 | 1.013 | – |
| Jaehnig et al. (2021) | 168.244 | -60.789 | 0.397 | -6.082 | 1.052 | – |
| Just et al. (2023) | 168.251 | -60.772 | – | – | – | – |
| Hunt & Reffert (2023) | 168.258 | -60.79 | 0.384 | -6.121 | 1.038 | – |
| Cavallo et al. (2024) | 168.263 | -60.784 | 0.384 | – | – | – |
| Celli et al. (2024) | 168.262 | -60.79 | – | – | – | – |
| Hunt & Reffert (2024) | 168.258 | -60.79 | 0.384 | -6.121 | 1.038 | – |
| Almeida et al. (2025) | 168.262 | -60.788 | – | – | – | – |
| UCC | 168.263 | -60.79 | 0.377 | -6.106 | 1.038 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.535, DM0=11.7, log_age_=7.2 |
| Dias et al. (2002) | E(B-V)=0.449, Dist=1651.0, Age=7.231 |
| Kharchenko et al. (2003) | E(B-V)=0.4, Dist=1639 |
| Kharchenko et al. (2005) | E(B-V)=0.45, Dist=1651, logt=7.55 |
| Piskunov et al. (2008) | E(B-V)=0.45, Dist=1651, logt=7.55, logMA=2.832 |
| Kharchenko et al. (2013) | E(B-V)=0.416, d=1660.0, logt=7.4 |
| Kharchenko et al. (2016) | E(B-V)=0.416, d=1660.0, logt=7.4 |
| Loktin & Popova (2017) | E(B-V)=0.449, Dist=1651, logt=7.231 |
| Cantat-Gaudin et al. (2018) | dmode=2564.1 |
| Soubiran et al. (2018) | dmode=2564.1 |
| Liu & Pang (2019) | Age=0.007, Z=0.5 |
| Cantat-Gaudin et al. (2020) | AVNN=1.3, DistPc=2638.0, AgeNN=7.42 |
| Dias et al. (2021) | Av=1.662, Dist=2420, logage=7.147, [Fe/H]=0.058 |
| Rain et al. (2021) | E(B-V)=0.44, Dist=2564.1, log(Age)=7.23, NBSS=0 |
| Jaehnig et al. (2021) | dmode=2.508 |
| Just et al. (2023) | logt=7.4, logmt=2.478 |
| Hunt & Reffert (2023) | AV50=1.424, diffAV50=2.013, MOD50=11.906, logAge50=7.338 |
| Cavallo et al. (2024) | AV50=1.55, dMod50=11.82, logAge50=7.24, [Fe/H]50=0.01 |
| Celli et al. (2024) | Age=26.3, Mc=906.5 |
| Hunt & Reffert (2024) | MassJ=956.648, MassTot=968.426 |
| Almeida et al. (2025) | AV=1.662, Dist=2420, logAge=7.147, MassRk=1134.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| DBSB 61 | 100.0 | 168.26 | -60.79 | 0.38 | -6.11 | 1.05 | – | 0.1 |