HSC 1042

Click to load Aladin Lite
0.32 UTI
0.37
CN
0.37
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.5 [pc], 1.8 [pc-2]
  • CN 0.37 Poorly populated
  • Cdens 0.37 Loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1042 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.34 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.34 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 26.122 61.303 0.156 -0.742 -0.177 –
Hu & Soubiran 2025 26.123 61.299 – – – –
Hunt & Reffert 2024 26.131 61.3 0.167 -0.72 -0.18 –
Cavallo et al. 2024 26.123 61.299 0.162 – – –
Hunt & Reffert 2023 26.131 61.3 0.167 -0.72 -0.18 –

💡 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 99999– 4.76 3.54 1.79 552 0.500 1091 – –
Hunt & Reffert 2024 4.76 3.54 1.79 552 – 1091(1) – –
Cavallo et al. 2024 3.28 3.52 – 676 0.500 – – –
Hunt & Reffert 2023 4.76 3.54 1.79 552 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3255 94.6 26.12 61.3 0.16 -0.75 -0.17 – 0.06

💡 Note: The % column shows the percentage of members that HSC 1042 shares with each listed object.

Visualization

â„šī¸