HXHWL 65
Summary
HXHWL 65 is a poorly populated, very dense object of high C3 quality. It is located at a close distance from the Sun, above the mid-plane. It is poorly studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2021) | 122.377 | -27.159 | 0.99 | -3.93 | 2.0 | – |
| Hunt & Reffert (2023) | 122.424 | -27.136 | 0.992 | -3.942 | 2.038 | 7.18 |
| Cavallo et al. (2024) | 122.409 | -27.131 | 0.997 | – | – | – |
| Hunt & Reffert (2024) | 122.424 | -27.136 | 0.992 | -3.942 | 2.038 | 7.18 |
| UCC | 122.413 | -27.151 | 1.006 | -3.955 | 2.026 | 8.093 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2021) | AG=0.2, m-M=10.1, logAge=8.2, Z=0.028 |
| Hunt & Reffert (2023) | AV50=0.078, diffAV50=0.193, MOD50=9.813, logAge50=8.679 |
| Cavallo et al. (2024) | AV50=0.0, dMod50=9.99, logAge50=8.57, [Fe/H]50=0.36 |
| Hunt & Reffert (2024) | MassJ=76.7146, MassTot=104.472 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWWDL 14423 | 94.3 | 122.41 | -27.15 | 1.01 | -3.96 | 2.03 | 8.57 | 0.01 |
