HSC 441

Click to load Aladin Lite
0.23 UTI
0.32
CN
0.82
Cdens
0.38
CC3
0.0
Clit
0.75
Cdup
Stellar density (N50/rad) 4.1 [N/pc2]
  • CN 0.32 Poorly populated
  • Cdens 0.82 Dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.75 Very likely unique

Overview

â„šī¸
HSC 441 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 292.537 18.304 0.781 -0.999 -5.454 13.075
Hunt & Reffert 2024 292.587 18.279 0.77 -1.064 -5.447 0.681
Cavallo et al. 2024 292.425 18.223 0.776 – – –
Hunt & Reffert 2023 292.587 18.279 0.77 -1.064 -5.447 0.681

💡 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– 1.33 3.25 2.75 8 -0.230 536 – –
Hunt & Reffert 2024 – – – – – 536(1) – –
Cavallo et al. 2024 1.41 3.13 – 8 -0.230 – – –
Hunt & Reffert 2023 1.25 3.37 2.75 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 12 25.0 292.58 18.34 0.64 -1.19 -5.57 -4.19 0.2
G3CC 69 18.8 292.32 17.95 0.78 -1.16 -5.21 -4.07 0.44

💡 Note: The % column shows the percentage of members that HSC 441 shares with each listed object.

Visualization

â„šī¸