Collinder 60
(NGC 1817; MWSC 484; OCL 463; FoF 0)
Summary
Collinder 60 is a very rich, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It is very well-studied in the literature.
This object shares a very small percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 78.062 | 16.69 | – | -1.79 | -2.17 | 65.31 |
| Chen et al. (2003) | 78.027 | 16.698 | – | – | – | – |
| Kharchenko et al. (2003) | 78.03 | 16.69 | – | 1.47 | -3.37 | – |
| Kharchenko et al. (2005) | 78.06 | 16.69 | – | -0.06 | -3.13 | – |
| Piskunov et al. (2007) | 78.056 | 16.693 | – | – | – | – |
| Kharchenko et al. (2007) | 78.06 | 16.69 | – | 0.23 | – | – |
| Piskunov et al. (2008) | 78.056 | 16.693 | – | – | – | – |
| Kharchenko et al. (2013) | 78.082 | 16.68 | – | 1.0 | -1.6 | 65.3 |
| Kharchenko et al. (2016) | 78.075 | 16.68 | – | – | – | – |
| Loktin & Popova (2017) | 78.06 | 16.691 | – | 0.084 | -0.323 | 65.3 |
| Cantat-Gaudin et al. (2018) | 78.139 | 16.696 | 0.551 | 0.485 | -0.89 | – |
| Bica et al. (2019) | 78.116 | 16.696 | – | – | – | – |
| Soubiran et al. (2018) | 78.139 | 16.696 | – | – | – | 66.07 |
| Liu & Pang (2019) | 78.138 | 16.71 | 0.549 | 0.516 | -0.888 | – |
| Cantat-Gaudin et al. (2020) | 78.139 | 16.696 | 0.551 | 0.485 | -0.89 | – |
| Dias et al. (2021) | 78.132 | 16.702 | 0.553 | 0.504 | -0.88 | 65.554 |
| Rain et al. (2021) | 78.139 | 16.696 | 0.551 | 0.485 | -0.89 | – |
| Jaehnig et al. (2021) | 78.136 | 16.686 | 0.582 | 0.482 | -0.883 | – |
| Just et al. (2023) | 78.075 | 16.68 | – | – | – | – |
| Cordoni et al. (2023) | 78.132 | 16.702 | 0.553 | 0.504 | -0.88 | – |
| Hunt & Reffert (2023) | 78.141 | 16.693 | 0.573 | 0.43 | -0.932 | 66.742 |
| Cavallo et al. (2024) | 78.134 | 16.697 | 0.572 | – | – | – |
| Hunt & Reffert (2024) | 78.141 | 16.693 | 0.573 | 0.43 | -0.932 | 66.742 |
| Zhang et al. (2024) | 78.141 | 16.693 | – | – | – | – |
| Almeida et al. (2025) | 78.132 | 16.702 | – | – | – | – |
| Carrasco-Varela et al. (2025) | 78.379 | 16.683 | – | – | – | – |
| Hu & Soubiran (2025) | 78.134 | 16.698 | – | – | – | – |
| UCC | 78.145 | 16.699 | 0.568 | 0.428 | -0.929 | 65.739 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.334, Dist=1972.0, Age=8.612, [Fe/H]=-0.16 |
| Chen et al. (2003) | E(B-V)=0.334, HDis=1972, Age=0.4, [Fe/H]_1=-0.26 |
| Kharchenko et al. (2003) | E(B-V)=0.33, Dist=1960 |
| Kharchenko et al. (2005) | E(B-V)=0.33, Dist=1972, logt=8.25 |
| Piskunov et al. (2007) | E(B-V)=0.33, Dist=1972, logt=8.25, logM=2.514 |
| Piskunov et al. (2008) | E(B-V)=0.33, Dist=1972, logt=8.25, logM=3.191, logMA=3.244 |
| Kharchenko et al. (2013) | E(B-V)=0.354, d=1504.0, logt=8.9, [Fe/H]=-0.14 |
| Kharchenko et al. (2016) | E(B-V)=0.354, d=1504.0, logt=8.9 |
| Loktin & Popova (2017) | E(B-V)=0.326, Dist=2004, logt=8.633 |
| Cantat-Gaudin et al. (2018) | dmode=1723.0 |
| Soubiran et al. (2018) | dmode=1723.0 |
| Liu & Pang (2019) | Age=1.41, Z=-0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=0.59, DistPc=1799.0, AgeNN=9.05 |
| Dias et al. (2021) | Av=0.722, Dist=1582, logage=9.092, [Fe/H]=-0.1 |
| Rain et al. (2021) | E(B-V)=0.33, Dist=1723.0, log(Age)=8.61, NBSS=3 |
| Jaehnig et al. (2021) | dmode=1.7 |
| Just et al. (2023) | logt=8.9, logmt=2.462 |
| Cordoni et al. (2023) | Av=0.722, Dist=10.996, logAge=9.092, [Fe/H]=-0.1, mass-single=1904.4, fbin-tot=0.222, fbss-MS=0.013 |
| Hunt & Reffert (2023) | AV50=0.341, diffAV50=0.506, MOD50=11.063, logAge50=9.124 |
| Cavallo et al. (2024) | AV50=0.65, dMod50=11.08, logAge50=9.07, [Fe/H]50=0.12 |
| Hunt & Reffert (2024) | MassJ=2712.84, MassTot=2712.84 |
| Zhang et al. (2024) | [Fe/H]ANN=-0.1702, [Fe/H]MCMC=-0.2006 |
| Almeida et al. (2025) | AV=0.722, Dist=1582, logAge=9.092, MassRk=1489.4 |
| Carrasco-Varela et al. (2025) | Av=0.722, Dist=1582, logAge=9.092, [Fe/H]=-0.1, NBSS=1, fBSS/MS=0.135 |
| Hu & Soubiran (2025) | MA22=-0.23, MA23f=-0.29, MA23g=-0.2, MZ23=-0.24, MK24=-0.21, MF24=-0.18 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| NGC 1807 | 2.9 | 77.79 | 16.55 | 0.54 | 0.45 | -0.94 | 65.36 | 0.04 |
