HSC 2945

Click to load Aladin Lite
0.45 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 6.4 [N/pc2]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2945 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, young 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.

Palma et al. (2025)
Part of multiple system G175, along with Trumpler_28 and Antalova_1.

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 265.567 -33.504 0.64 1.336 0.458 -20.46
Hunt & Reffert 2024 265.594 -33.495 0.645 1.318 0.456 1.617
Cavallo et al. 2024 265.559 -33.516 0.643 – – –
Hunt & Reffert 2023 265.594 -33.495 0.645 1.318 0.456 1.617

💡 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– 1.405 3.155 1.64 81 -0.760 465 – –
Hunt & Reffert 2024 – – – – – 465(1) – –
Cavallo et al. 2024 1.37 3.43 – 89 -0.760 – – –
Hunt & Reffert 2023 1.44 2.88 1.64 73 – – – –

(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 3799 96.1 265.56 -33.51 0.65 1.32 0.43 -20.46 0.06

💡 Note: The % column shows the percentage of members that HSC 2945 shares with each listed object.

Visualization

â„šī¸