UBC 1090
Summary
UBC 1090 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
This object shares a significant percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Castro-Ginard et al. (2022) | 302.49 | 34.31 | 0.4 | -0.67 | -2.33 | -3.23 |
| Hunt & Reffert (2023) | 302.497 | 34.337 | 0.397 | -0.67 | -2.365 | -4.354 |
| Cavallo et al. (2024) | 302.485 | 34.32 | 0.397 | – | – | – |
| Hunt & Reffert (2024) | 302.497 | 34.337 | 0.397 | -0.67 | -2.365 | -4.354 |
| UCC | 302.494 | 34.329 | 0.399 | -0.655 | -2.353 | -4.351 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Castro-Ginard et al. (2022) | AV=2.106, Dist=2513, logAge=8.565 |
| Hunt & Reffert (2023) | AV50=2.621, diffAV50=1.722, MOD50=11.795, logAge50=8.574 |
| Cavallo et al. (2024) | AV50=3.08, dMod50=11.69, logAge50=8.34, [Fe/H]50=-0.15 |
| Hunt & Reffert (2024) | MassJ=383.193, MassTot=410.176 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 376 | 71.4 | 302.5 | 34.33 | 0.4 | -0.66 | -2.35 | -4.35 | 0.0 |
