NGC 2467
Summary
NGC 2467 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.
This object shares a large percentage of members with a later reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 118.08 | -26.442 | – | – | – | – |
| Dias et al. (2002) | 118.108 | -26.437 | – | -3.65 | 2.68 | 58.24 |
| Chen et al. (2003) | 118.088 | -26.363 | – | -5.82 | 1.63 | 66.0 |
| Piskunov et al. (2008) | 118.059 | -26.437 | – | – | – | – |
| Loktin & Popova (2017) | 118.11 | -26.436 | – | – | – | 55.8 |
| Jaehnig et al. (2021) | 118.18 | -26.374 | 0.191 | -2.554 | 2.578 | – |
| Hunt & Reffert (2023) | 117.997 | -26.411 | 0.216 | -1.49 | 2.453 | 77.739 |
| Cavallo et al. (2024) | 117.925 | -26.383 | 0.216 | – | – | – |
| Hunt & Reffert (2024) | 117.997 | -26.411 | 0.216 | -1.49 | 2.453 | 77.739 |
| UCC | 117.969 | -26.408 | 0.214 | -1.486 | 2.45 | 77.88 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.298, DM0=10.5, log_age_=7.7 |
| Dias et al. (2002) | E(B-V)=0.338, Dist=1355.0, Age=7.103 |
| Chen et al. (2003) | HDis=1355, Age=0.01 |
| Piskunov et al. (2008) | E(B-V)=0.34, Dist=1355, logt=8.05, logMA=2.796 |
| Loktin & Popova (2017) | E(B-V)=0.338, Dist=1355, logt=7.103 |
| Jaehnig et al. (2021) | dmode=5.169 |
| Hunt & Reffert (2023) | AV50=0.734, diffAV50=1.192, MOD50=13.295, logAge50=8.394 |
| Cavallo et al. (2024) | AV50=0.47, dMod50=12.9, logAge50=8.46, [Fe/H]50=0.43 |
| Hunt & Reffert (2024) | MassJ=101.727, MassTot=180.760 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 1615 | 76.0 | 117.95 | -26.34 | 0.22 | -1.48 | 2.44 | 77.88 | 0.03 |