HXHWL 49
0.49
UTI
0.42
CN
0.79
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
7.2 [arcmin]
- CN 0.42 Poorly populated
- Cdens 0.79 Dense
- CC3 0.62 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
HXHWL 49 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close 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 large 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 | 77.707 | 36.371 | 0.641 | 1.108 | -4.011 | -6.011 |
| Zhang et al. | 2024 | 77.703 | 36.365 | â | â | â | â |
| Hunt & Reffert | 2024 | 77.703 | 36.365 | 0.644 | 1.118 | -4.02 | -5.958 |
| Cavallo et al. | 2024 | 77.731 | 36.363 | 0.642 | â | â | â |
| Hunt & Reffert | 2023 | 77.703 | 36.365 | 0.644 | 1.118 | -4.02 | -5.958 |
| He et al. | 2021 | 77.708 | 36.357 | 0.6 | 1.15 | -3.97 | 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 | -0.215* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 161* | â | â |
| Cavallo et al. | 2024 | 1.57 | 1.26 | â | 98 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 1.46 | 1.04 | 0.82 | 120 | â | â | â | â |
| He et al. | 2021 | 1.51 | 1.44 | â | 151 | 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.