HXHWL 35
0.43
UTI
0.32
CN
0.6
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
5.5 [arcmin]
- CN 0.32 Poorly populated
- Cdens 0.6 Moderately dense
- CC3 0.62 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
HXHWL 35 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 71.989 | 44.01 | 0.491 | 1.409 | -2.16 | â |
| Zhang et al. | 2024 | 72.014 | 43.967 | â | â | â | â |
| Hunt & Reffert | 2024 | 72.014 | 43.967 | 0.492 | 1.394 | -2.164 | â |
| Cavallo et al. | 2024 | 71.965 | 44.022 | 0.496 | â | â | â |
| Hunt & Reffert | 2023 | 72.014 | 43.967 | 0.492 | 1.394 | -2.164 | â |
| He et al. | 2021 | 72.022 | 44.0 | 0.52 | 1.43 | -2.11 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.150* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 217* | â | â |
| Cavallo et al. | 2024 | 2.02 | 1.09 | â | 54 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 1.88 | 1.02 | 0.48 | 109 | â | â | â | â |
| He et al. | 2021 | 2.00 | 1.20 | â | 275 | 0.457 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.