NGC 2362
(FoF 671)
Summary
NGC 2362 is a very rich, very dense object of 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.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 109.671 | -24.955 | – | – | – | – |
| Dias et al. (2002) | 109.671 | -24.955 | – | -2.29 | 3.03 | 36.43 |
| Chen et al. (2003) | 109.729 | -24.951 | – | -2.29 | 3.03 | 42.2 |
| Piskunov et al. (2007) | 109.66 | -24.984 | – | – | – | – |
| Piskunov et al. (2008) | 109.66 | -24.984 | – | – | – | – |
| Kharchenko et al. (2012) | 109.68 | -24.96 | – | -2.6 | 2.34 | – |
| Loktin & Popova (2017) | 109.68 | -24.96 | – | -3.539 | 1.159 | 29.5 |
| Cantat-Gaudin et al. (2018) | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | – |
| Soubiran et al. (2018) | 109.671 | -24.954 | – | – | – | 28.86 |
| Dias et al. (2019) | 109.671 | 24.954 | 0.742 | -2.791 | 2.953 | 28.86 |
| Liu & Pang (2019) | 109.666 | -24.931 | 0.748 | -2.769 | 2.952 | – |
| Cantat-Gaudin et al. (2020) | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | – |
| Dias et al. (2021) | 109.672 | -24.949 | 0.743 | -2.779 | 2.95 | – |
| Rain et al. (2021) | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | – |
| Jaehnig et al. (2021) | 109.673 | -24.933 | 0.786 | -2.783 | 2.916 | – |
| Hunt & Reffert (2023) | 109.672 | -24.952 | 0.774 | -2.763 | 2.974 | 42.196 |
| Cavallo et al. (2024) | 109.693 | -24.967 | 0.778 | – | – | – |
| Celli et al. (2024) | 109.671 | -24.954 | – | – | – | – |
| Hunt & Reffert (2024) | 109.672 | -24.952 | 0.774 | -2.763 | 2.974 | 42.196 |
| Almeida et al. (2025) | 109.672 | -24.949 | – | – | – | – |
| UCC | 109.68 | -24.953 | 0.767 | -2.778 | 2.987 | 34.408 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.11, DM0=10.53, log_age_=7.0 |
| Dias et al. (2002) | E(B-V)=0.1, Dist=1480.0, Age=6.7 |
| Chen et al. (2003) | HDis=1389, Age=0.0 |
| Piskunov et al. (2007) | E(B-V)=0.1, Dist=1389, logt=6.64, logM=1.852 |
| Piskunov et al. (2008) | E(B-V)=0.1, Dist=1389, logt=6.64, logM=2.504, logMA=3.002 |
| Kharchenko et al. (2012) | e_bv=0.167, distance=1375, log_age=6.64 |
| Loktin & Popova (2017) | E(B-V)=0.097, Dist=1386, logt=6.917 |
| Cantat-Gaudin et al. (2018) | dmode=1296.5 |
| Soubiran et al. (2018) | dmode=1296.5 |
| Dias et al. (2019) | E(B-V)=0.17, Dist=1285, logAge=6.872, Z=0.005 |
| Liu & Pang (2019) | Age=0.008, Z=0.5 |
| Cantat-Gaudin et al. (2020) | AVNN=0.37, DistPc=1341.0, AgeNN=6.76 |
| Dias et al. (2021) | Av=0.43, Dist=1233, logage=7.156, [Fe/H]=-0.104 |
| Rain et al. (2021) | E(B-V)=0.1, Dist=1296.5, log(Age)=6.7, NBSS=0 |
| Jaehnig et al. (2021) | dmode=1.268 |
| Hunt & Reffert (2023) | AV50=0.384, diffAV50=1.346, MOD50=10.437, logAge50=6.842 |
| Cavallo et al. (2024) | AV50=0.3, dMod50=10.37, logAge50=6.74, [Fe/H]50=0.03 |
| Celli et al. (2024) | Age=5.8, Mc=591.7 |
| Hunt & Reffert (2024) | MassJ=388.737, MassTot=388.639 |
| Almeida et al. (2025) | AV=0.43, Dist=1233, logAge=7.156, MassRk=546.8 |
Search coordinates in Bayestar19