HSC 749

Click to load Aladin Lite
0.11 UTI
0.25
CN
0.09
Cdens
0.25
CC3
0.25
Clit
0.52
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.52 Likely unique

Overview

â„šī¸
HSC 749 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 87 along with CWNU_1066.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 6.058 2.707 8.226 18.258 -14.783 12.493
Zhang et al. 2024 358.47 3.455 – – – –
Cavallo et al. 2024 5.95 2.012 8.109 – – –
Hunt & Reffert 2023 358.47 3.455 8.128 18.061 -13.839 16.442

💡 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– 0.13 0.1 0.45 226 0.102 – – –
Liu et al. 2025 0.16 0.10 – 83 – – – –
Zhang et al. 2024 – – – – 0.034(1) – – –
Cavallo et al. 2024 0.13 0.50 – 309 0.170 – – –
Hunt & Reffert 2023 0.12 0.07 0.45 226 – – – –

(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 1077 48.0 9.5 1.9 8.43 17.55 -14.39 15.68 0.17

💡 Note: The % column shows the percentage of members that HSC 749 shares with each listed object.

Visualization

â„šī¸