IC 2395
(FoF 2288)
Summary
IC 2395 is a very rich, very dense object of very high C3 quality. It is located at a close distance from the Sun, near 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) | 130.629 | -48.1 | – | – | – | – |
| Dias et al. (2002) | 130.625 | -48.113 | – | -6.69 | 5.87 | 8.99 |
| Chen et al. (2003) | 130.345 | -48.212 | – | -3.6 | 2.21 | 0.5 |
| Piskunov et al. (2007) | 130.621 | -48.107 | – | – | – | – |
| Piskunov et al. (2008) | 130.621 | -48.107 | – | – | – | – |
| Kharchenko et al. (2012) | 130.65 | -48.133 | – | -5.26 | 3.97 | – |
| Loktin & Popova (2017) | 130.62 | -48.112 | – | -4.424 | 6.17 | 13.2 |
| Cantat-Gaudin et al. (2018) | 130.531 | -48.09 | 1.379 | -4.464 | 3.293 | – |
| Soubiran et al. (2018) | 130.531 | -48.09 | – | – | – | 17.66 |
| Dias et al. (2019) | 130.625 | -48.113 | 1.382 | -4.385 | 3.199 | 23.197 |
| Liu & Pang (2019) | 130.484 | -48.064 | 1.386 | -4.441 | 3.231 | – |
| Cantat-Gaudin et al. (2020) | 130.531 | -48.09 | 1.379 | -4.464 | 3.293 | – |
| Dias et al. (2021) | 130.471 | -48.072 | 1.375 | -4.463 | 3.258 | 19.065 |
| Rain et al. (2021) | 130.531 | -48.09 | 1.379 | -4.464 | 3.293 | – |
| Jaehnig et al. (2021) | 130.586 | -48.137 | 1.409 | -4.393 | 3.193 | – |
| He et al. (2022) | 130.466 | -48.053 | 1.409 | -4.464 | 3.365 | – |
| Hunt & Reffert (2023) | 130.62 | -48.134 | 1.404 | -4.487 | 3.371 | 23.948 |
| Cavallo et al. (2024) | 130.325 | -47.976 | 1.407 | – | – | – |
| Celli et al. (2024) | 130.531 | -48.09 | – | – | – | – |
| Hunt & Reffert (2024) | 130.62 | -48.134 | 1.404 | -4.487 | 3.371 | 23.948 |
| Alfonso et al. (2024) | 130.471 | -48.01 | 1.377 | -4.506 | 3.415 | – |
| Almeida et al. (2025) | 130.471 | -48.072 | – | – | – | – |
| UCC | 130.523 | -48.1 | 1.403 | -4.443 | 3.32 | 22.316 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.073, DM0=9.1, log_age_=7.3 |
| Dias et al. (2002) | E(B-V)=0.09, Dist=800.0, Age=6.8, [Fe/H]=0.0 |
| Chen et al. (2003) | HDis=705, Age=0.01 |
| Piskunov et al. (2007) | E(B-V)=0.07, Dist=709, logt=7.08, logM=1.877 |
| Piskunov et al. (2008) | E(B-V)=0.07, Dist=709, logt=7.08, logM=2.246, logMA=2.503 |
| Kharchenko et al. (2012) | e_bv=0.146, distance=701, log_age=7.27, metallicity=0.0 |
| Loktin & Popova (2017) | E(B-V)=0.066, Dist=711, logt=7.22 |
| Cantat-Gaudin et al. (2018) | dmode=710.5 |
| Soubiran et al. (2018) | dmode=710.5 |
| Dias et al. (2019) | E(B-V)=0.15, Dist=817, logAge=7.051, Z=0.01 |
| Liu & Pang (2019) | Age=0.011, Z=-0.75 |
| Cantat-Gaudin et al. (2020) | AVNN=0.51, DistPc=702.0, AgeNN=7.31 |
| Dias et al. (2021) | Av=0.475, Dist=710, logage=7.149, [Fe/H]=-0.007 |
| Rain et al. (2021) | E(B-V)=0.09, Dist=710.5, log(Age)=6.8, NBSS=0 |
| Jaehnig et al. (2021) | dmode=0.71 |
| He et al. (2022) | A0=0.25, logAge=6.9 |
| Hunt & Reffert (2023) | AV50=0.305, diffAV50=1.423, MOD50=9.191, logAge50=6.833 |
| Cavallo et al. (2024) | AV50=0.75, dMod50=9.32, logAge50=6.41, [Fe/H]50=-0.37 |
| Celli et al. (2024) | Age=20.4, Mc=388.9 |
| Hunt & Reffert (2024) | MassJ=782.053, MassTot=866.445 |
| Alfonso et al. (2024) | AV=0.50732, MOD=9.23016, logAge=7.15887, Z=-0.0078 |
| Almeida et al. (2025) | AV=0.475, Dist=710, logAge=7.149, MassRk=674.9 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0489 | 3.1 | 129.93 | -47.6 | 1.42 | -4.65 | 3.67 | 18.42 | 0.09 |