HSC 37
0.25
UTI
0.3
CN
0.2
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
1.0 [N/pc2]
- CN 0.3 Poorly populated
- Cdens 0.2 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
HSC 37 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a very large* distance, well above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
(*): The parallax distance estimate (~10.02 kpc) differs significantly from the median photometric distance (~6.83 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 264.357 | -24.41 | 0.1 | -3.146 | -4.567 | 112.099 |
| Hunt & Reffert | 2024 | 264.355 | -24.406 | 0.097 | -3.173 | -4.548 | 21.863 |
| Cavallo et al. | 2024 | 264.35 | -24.433 | 0.096 | â | â | â |
| Hunt & Reffert | 2023 | 264.355 | -24.406 | 0.097 | -3.173 | -4.548 | 21.863 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 6.83 | 4.265 | 2.85 | 26 | -0.150 | 2060 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2060(1) | â | â |
| Cavallo et al. | 2024 | 4.47 | 4.20 | â | 35 | -0.150 | â | â | â |
| Hunt & Reffert | 2023 | 9.19 | 4.33 | 2.85 | 18 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Wood sample.