Collinder 413
(NGC 6871; MWSC 3253; OCL 148; FoF 493)
Summary
Collinder 413 is a rich, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, above 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 |
|---|---|---|---|---|---|---|
| Dambis (1999) | 301.496 | 35.777 | – | – | – | – |
| Dias et al. (2002) | 301.496 | 35.777 | – | -3.26 | -5.15 | -108.01 |
| Chen et al. (2003) | 301.418 | 35.764 | – | -3.23 | -6.93 | -7.7 |
| Kharchenko et al. (2003) | 301.47 | 35.77 | – | -3.68 | -7.82 | – |
| Kharchenko et al. (2005) | 301.5 | 35.78 | – | -3.65 | -7.19 | -10.54 |
| Piskunov et al. (2007) | 301.486 | 35.776 | – | – | – | – |
| Kharchenko et al. (2007) | 301.5 | 35.78 | – | 0.23 | – | -10.54 |
| Piskunov et al. (2008) | 301.486 | 35.776 | – | – | – | – |
| Kharchenko et al. (2013) | 301.5 | 35.77 | – | -3.39 | -6.82 | -10.5 |
| Kharchenko et al. (2016) | 301.494 | 35.767 | – | – | – | – |
| Loktin & Popova (2017) | 301.5 | 35.777 | – | -2.676 | -5.114 | -10.5 |
| Cantat-Gaudin et al. (2018) | 301.548 | 35.765 | 0.514 | -3.129 | -6.437 | – |
| Bica et al. (2019) | 301.497 | 35.77 | – | – | – | – |
| Soubiran et al. (2018) | 301.548 | 35.765 | – | – | – | 4.38 |
| Liu & Pang (2019) | 301.488 | 35.791 | 0.522 | -3.152 | -6.444 | – |
| Cantat-Gaudin et al. (2020) | 301.548 | 35.765 | 0.514 | -3.129 | -6.437 | – |
| Dias et al. (2021) | 301.586 | 35.77 | 0.516 | -3.12 | -6.444 | – |
| Rain et al. (2021) | 301.548 | 35.765 | 0.514 | -3.129 | -6.437 | – |
| Jaehnig et al. (2021) | 301.518 | 35.769 | 0.544 | -3.121 | -6.426 | – |
| Just et al. (2023) | 301.494 | 35.767 | – | – | – | – |
| Hunt & Reffert (2023) | 301.49 | 35.776 | 0.513 | -3.092 | -6.446 | -0.99 |
| Cavallo et al. (2024) | 301.593 | 35.753 | 0.514 | – | – | – |
| Celli et al. (2024) | 301.548 | 35.765 | – | – | – | – |
| Hunt & Reffert (2024) | 301.49 | 35.776 | 0.513 | -3.092 | -6.446 | -0.99 |
| Zhang et al. (2024) | 301.49 | 35.776 | – | – | – | – |
| Almeida et al. (2025) | 301.586 | 35.77 | – | – | – | – |
| UCC | 301.511 | 35.764 | 0.515 | -3.108 | -6.458 | 0.538 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.447, DM0=10.9, log_age_=7.0 |
| Dias et al. (2002) | E(B-V)=0.443, Dist=1574.0, Age=6.958 |
| Chen et al. (2003) | HDis=1574, Age=0.0 |
| Kharchenko et al. (2003) | E(B-V)=0.44, Dist=1574 |
| Kharchenko et al. (2005) | E(B-V)=0.44, Dist=1574, logt=6.99 |
| Piskunov et al. (2007) | E(B-V)=0.44, Dist=1574, logt=6.99, logM=2.064 |
| Piskunov et al. (2008) | E(B-V)=0.44, Dist=1574, logt=6.99, logM=2.698, logMA=3.062 |
| Kharchenko et al. (2013) | E(B-V)=0.416, d=1791.0, logt=6.99 |
| Kharchenko et al. (2016) | E(B-V)=0.416, d=1791.0, logt=6.99 |
| Loktin & Popova (2017) | E(B-V)=0.441, Dist=1616, logt=6.975 |
| Cantat-Gaudin et al. (2018) | dmode=1841.0 |
| Soubiran et al. (2018) | dmode=1841.0 |
| Liu & Pang (2019) | Age=0.007, Z=0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=1.19, DistPc=1720.0, AgeNN=6.74 |
| Dias et al. (2021) | Av=1.439, Dist=1741, logage=7.064, [Fe/H]=0.104 |
| Rain et al. (2021) | E(B-V)=0.44, Dist=1841.0, log(Age)=6.95, NBSS=0 |
| Jaehnig et al. (2021) | dmode=1.824 |
| Just et al. (2023) | logt=6.99, logmt=2.936 |
| Hunt & Reffert (2023) | AV50=1.331, diffAV50=1.666, MOD50=11.315, logAge50=6.89 |
| Cavallo et al. (2024) | AV50=1.43, dMod50=11.29, logAge50=6.89, [Fe/H]50=0.0 |
| Celli et al. (2024) | Age=5.5, Mc=2822.3 |
| Hunt & Reffert (2024) | MassJ=1601.14, MassTot=1625.91 |
| Zhang et al. (2024) | [Fe/H]ANN=-0.0503, [Fe/H]MCMC=-0.0078 |
| Almeida et al. (2025) | AV=1.439, Dist=1741, logAge=7.064, MassRk=2423.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0102 | 6.6 | 301.71 | 35.64 | 0.53 | -3.1 | -6.61 | -17.95 | 0.08 |