NGC 869
(MWSC 175)
Summary
NGC 869 is a very rich, very dense object of very high C3 quality. It is located at a moderate 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 |
|---|---|---|---|---|---|---|
| Dambis (1999) | 34.75 | 57.128 | – | – | – | – |
| Dias et al. (2002) | 34.75 | 57.128 | – | -0.92 | -1.66 | -42.84 |
| Chen et al. (2003) | 34.719 | 57.178 | – | -0.92 | -1.66 | -53.0 |
| Kharchenko et al. (2003) | 34.77 | 57.15 | – | -0.56 | 1.46 | – |
| Kharchenko et al. (2005) | 34.77 | 57.15 | – | -0.49 | -0.9 | -39.82 |
| Kharchenko et al. (2007) | 34.75 | 57.13 | – | 1.75 | – | -39.84 |
| Piskunov et al. (2008) | 34.759 | 57.149 | – | – | – | – |
| Kharchenko et al. (2012) | 34.74 | 57.145 | – | -2.81 | 0.05 | -41.77 |
| Kharchenko et al. (2013) | 34.74 | 57.145 | – | -2.81 | 0.05 | -41.8 |
| Kharchenko et al. (2016) | 34.728 | 57.143 | – | – | – | – |
| Loktin & Popova (2017) | 34.755 | 57.129 | – | -0.738 | -0.15 | -41.8 |
| Cantat-Gaudin et al. (2018) | 34.741 | 57.134 | 0.399 | -0.689 | -1.082 | – |
| Soubiran et al. (2018) | 34.741 | 57.134 | – | – | – | -62.82 |
| Cantat-Gaudin et al. (2020) | 34.741 | 57.134 | 0.399 | -0.689 | -1.082 | – |
| Dias et al. (2021) | 34.744 | 57.136 | 0.4 | -0.682 | -1.077 | – |
| Rain et al. (2021) | 34.741 | 57.134 | 0.399 | -0.689 | -1.082 | – |
| Jaehnig et al. (2021) | 35.09 | 57.142 | 0.424 | -0.652 | -1.079 | – |
| Just et al. (2023) | 34.728 | 57.143 | – | – | – | – |
| Hunt & Reffert (2023) | 34.766 | 57.14 | 0.404 | -0.654 | -1.143 | -67.639 |
| Cavallo et al. (2024) | 34.735 | 57.132 | 0.403 | – | – | – |
| Celli et al. (2024) | 34.741 | 57.134 | – | – | – | – |
| Hunt & Reffert (2024) | 34.766 | 57.14 | 0.404 | -0.654 | -1.143 | -67.639 |
| Zhang et al. (2024) | 34.766 | 57.14 | – | – | – | – |
| Almeida et al. (2025) | 34.744 | 57.136 | – | – | – | – |
| UCC | 34.751 | 57.138 | 0.403 | -0.664 | -1.13 | -50.337 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.566, DM0=11.36, log_age_=6.5 |
| Dias et al. (2002) | E(B-V)=0.575, Dist=2079.0, Age=7.069, [Fe/H]=-0.3 |
| Chen et al. (2003) | HDis=2079, Age=0.01 |
| Kharchenko et al. (2003) | E(B-V)=0.58, Dist=2079 |
| Kharchenko et al. (2005) | E(B-V)=0.48, Dist=2079, logt=7.28 |
| Piskunov et al. (2008) | E(B-V)=0.48, Dist=2079, logt=7.28, logMA=6.022 |
| Kharchenko et al. (2012) | E(B-V)=0.521, d=2300.0, logt=7.28, [Fe/H]=-0.3 |
| Kharchenko et al. (2013) | E(B-V)=0.521, d=2300.0, logt=7.28, [Fe/H]=-0.3 |
| Kharchenko et al. (2016) | E(B-V)=0.521, d=2300.0, logt=7.28 |
| Loktin & Popova (2017) | E(B-V)=0.57, Dist=2094, logt=7.074 |
| Cantat-Gaudin et al. (2018) | dmode=2336.3 |
| Soubiran et al. (2018) | dmode=2336.3 |
| Cantat-Gaudin et al. (2020) | AVNN=1.69, DistPc=2197.0, AgeNN=7.18 |
| Dias et al. (2021) | Av=1.749, Dist=2246, logage=7.11, [Fe/H]=-0.1 |
| Rain et al. (2021) | E(B-V)=0.57, Dist=2336.3, log(Age)=7.06, NBSS=0 |
| Jaehnig et al. (2021) | dmode=2.394 |
| Just et al. (2023) | logt=7.28, logmt=3.893 |
| Hunt & Reffert (2023) | AV50=1.577, diffAV50=0.806, MOD50=11.864, logAge50=7.26 |
| Cavallo et al. (2024) | AV50=1.77, dMod50=12.12, logAge50=7.18, [Fe/H]50=0.08 |
| Celli et al. (2024) | Age=15.1, Mc=3678.7 |
| Hunt & Reffert (2024) | MassJ=2402.39, MassTot=2402.39 |
| Zhang et al. (2024) | [Fe/H]ANN=-0.0742, [Fe/H]MCMC=-0.0403 |
| Almeida et al. (2025) | AV=1.749, Dist=2246, logAge=7.11, MassRk=4596.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0247 | 0.6 | 34.61 | 56.85 | 0.38 | -0.62 | -1.18 | – | 0.16 |
