Czernik 25
(FSR 0987; SAI 63; MWSC 795; OCL 493; MWSC 804; FoF 29)
Summary
Czernik 25 is a rich, very dense object of 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.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 93.275 | 6.983 | – | -0.25 | -0.87 | – |
| Froebrich et al. (2007) | 93.446 | 6.95 | – | – | – | – |
| Glushkova et al. (2010) | 93.435 | 6.949 | – | – | – | – |
| Kharchenko et al. (2013) | 93.423 | 6.953 | – | 0.22 | 0.22 | – |
| Kharchenko et al. (2016) | 93.416 | 6.955 | – | – | – | – |
| Loktin & Popova (2017) | 93.42 | 6.954 | – | 0.188 | -0.56 | – |
| Cantat-Gaudin et al. (2018) | 93.432 | 6.953 | 0.438 | -0.222 | 0.252 | – |
| Bica et al. (2019) | 93.423 | 6.96 | – | – | – | – |
| Soubiran et al. (2018) | 93.432 | 6.953 | – | – | – | 42.79 |
| Bossini et al. (2019) | 93.432 | 6.953 | – | – | – | – |
| Liu & Pang (2019) | 93.441 | 6.941 | 0.445 | -0.208 | 0.244 | – |
| Cantat-Gaudin et al. (2020) | 93.432 | 6.953 | 0.438 | -0.222 | 0.252 | – |
| Dias et al. (2021) | 93.431 | 6.954 | 0.44 | -0.226 | 0.255 | – |
| Just et al. (2023) | 93.416 | 6.955 | – | – | – | – |
| Hunt & Reffert (2023) | 93.431 | 6.951 | 0.444 | -0.242 | 0.243 | 40.317 |
| Cavallo et al. (2024) | 93.432 | 6.939 | 0.442 | – | – | – |
| Hunt & Reffert (2024) | 93.431 | 6.951 | 0.444 | -0.242 | 0.243 | 40.317 |
| Zhang et al. (2024) | 93.431 | 6.951 | – | – | – | – |
| Almeida et al. (2025) | 93.431 | 6.954 | – | – | – | – |
| Hu & Soubiran (2025) | 93.432 | 6.939 | – | – | – | – |
| UCC | 93.427 | 6.946 | 0.445 | -0.244 | 0.234 | 43.943 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.58, Dist=1980.0, Age=8.11 |
| Glushkova et al. (2010) | E(B-V)=0.37, Dist=1910.0, Age=8.65 |
| Kharchenko et al. (2013) | E(B-V)=0.625, d=1861.0, logt=8.52 |
| Kharchenko et al. (2016) | E(B-V)=0.625, d=1861.0, logt=8.52 |
| Loktin & Popova (2017) | E(B-V)=0.582, Dist=6163, logt=8.92 |
| Cantat-Gaudin et al. (2018) | dmode=2141.9 |
| Soubiran et al. (2018) | dmode=2141.9 |
| Bossini et al. (2019) | AV=1.463, Dist=12.128, logA=8.56, Fe/H=0.0 |
| Liu & Pang (2019) | Age=0.933, Z=0.0 |
| Cantat-Gaudin et al. (2020) | AVNN=1.01, DistPc=2167.0, AgeNN=8.87 |
| Dias et al. (2021) | Av=1.431, Dist=1910, logage=8.802, [Fe/H]=-0.02 |
| Just et al. (2023) | logt=8.52, logmt=2.3 |
| Hunt & Reffert (2023) | AV50=1.21, diffAV50=1.168, MOD50=11.555, logAge50=8.73 |
| Cavallo et al. (2024) | AV50=1.58, dMod50=11.66, logAge50=8.75, [Fe/H]50=0.12 |
| Hunt & Reffert (2024) | MassJ=1057.85, MassTot=1072.78 |
| Zhang et al. (2024) | [Fe/H]ANN=0.12655, [Fe/H]MCMC=0.14753 |
| Almeida et al. (2025) | AV=1.431, Dist=1910, logAge=8.802, MassRk=529.8 |
| Hu & Soubiran (2025) | MA22=-0.15, MA23f=-0.36, MA23g=-0.08, MZ23=-0.19, MK24=-0.24, MF24=-0.17 |
Search coordinates in Bayestar19