NGC 3572
(MWSC 1906)
Summary
NGC 3572 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 small percentage of members with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 167.596 | -60.248 | – | – | – | – |
| Dias et al. (2002) | 167.596 | -60.248 | – | -4.37 | -0.96 | -4.0 |
| Kharchenko et al. (2003) | 167.61 | -60.25 | – | -9.7 | -1.02 | – |
| Kharchenko et al. (2005) | 167.61 | -60.25 | – | -10.55 | 1.25 | -9.5 |
| Kharchenko et al. (2007) | 167.59 | -60.25 | – | 0.11 | – | -8.47 |
| Piskunov et al. (2008) | 167.612 | -60.243 | – | – | – | – |
| Kharchenko et al. (2013) | 167.602 | -60.25 | – | -9.19 | 2.31 | -8.0 |
| Kharchenko et al. (2016) | 167.596 | -60.246 | – | – | – | – |
| Loktin & Popova (2017) | 167.595 | -60.248 | – | -4.37 | -0.96 | -8.0 |
| Cantat-Gaudin et al. (2018) | 167.64 | -60.294 | 0.376 | -6.261 | 1.893 | – |
| Soubiran et al. (2018) | 167.64 | -60.294 | – | – | – | 0.92 |
| Cantat-Gaudin et al. (2020) | 167.64 | -60.294 | 0.376 | -6.261 | 1.893 | – |
| Dias et al. (2021) | 167.633 | -60.302 | 0.383 | -6.266 | 1.904 | – |
| Rain et al. (2021) | 167.64 | -60.294 | 0.376 | -6.261 | 1.893 | – |
| Jaehnig et al. (2021) | 167.646 | -60.293 | 0.409 | -6.204 | 1.921 | – |
| Just et al. (2023) | 167.596 | -60.246 | – | – | – | – |
| Hunt & Reffert (2023) | 167.625 | -60.28 | 0.373 | -6.253 | 1.949 | -4.931 |
| Cavallo et al. (2024) | 167.639 | -60.302 | 0.371 | – | – | – |
| Celli et al. (2024) | 167.64 | -60.294 | – | – | – | – |
| Hunt & Reffert (2024) | 167.625 | -60.28 | 0.373 | -6.253 | 1.949 | -4.931 |
| Almeida et al. (2025) | 167.633 | -60.302 | – | – | – | – |
| UCC | 167.655 | -60.311 | 0.381 | -6.245 | 1.904 | -4.918 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.44, DM0=11.9, log_age_=6.5 |
| Dias et al. (2002) | E(B-V)=0.389, Dist=1995.0, Age=6.891 |
| Kharchenko et al. (2003) | E(B-V)=0.37, Dist=1995 |
| Kharchenko et al. (2005) | E(B-V)=0.34, Dist=2004, logt=6.88 |
| Piskunov et al. (2008) | E(B-V)=0.34, Dist=2004, logt=6.88, logMA=2.631 |
| Kharchenko et al. (2013) | E(B-V)=0.364, d=1997.0, logt=6.925 |
| Kharchenko et al. (2016) | E(B-V)=0.364, d=1997.0, logt=6.925 |
| Loktin & Popova (2017) | E(B-V)=0.387, Dist=2004, logt=6.896 |
| Cantat-Gaudin et al. (2018) | dmode=2470.4 |
| Soubiran et al. (2018) | dmode=2470.4 |
| Cantat-Gaudin et al. (2020) | AVNN=1.53, DistPc=2455.0, AgeNN=6.68 |
| Dias et al. (2021) | Av=1.435, Dist=2276, logage=6.811, [Fe/H]=0.071 |
| Rain et al. (2021) | E(B-V)=0.38, Dist=2470.4, log(Age)=6.89, NBSS=0 |
| Jaehnig et al. (2021) | dmode=2.456 |
| Just et al. (2023) | logt=6.925, logmt=2.21 |
| Hunt & Reffert (2023) | AV50=1.292, diffAV50=1.501, MOD50=11.921, logAge50=6.687 |
| Cavallo et al. (2024) | AV50=1.42, dMod50=11.75, logAge50=6.58, [Fe/H]50=-0.18 |
| Celli et al. (2024) | Age=4.8, Mc=542.8 |
| Hunt & Reffert (2024) | MassJ=502.358, MassTot=502.358 |
| Almeida et al. (2025) | AV=1.435, Dist=2276, logAge=6.811, MassRk=659.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch 227 | 16.4 | 167.49 | -60.31 | 0.37 | -6.22 | 1.85 | -28.47 | 0.15 |
| Hogg 10 | 14.8 | 167.68 | -60.41 | 0.39 | -6.2 | 1.79 | -10.87 | 0.79 |