HSC 1428

Click to load Aladin Lite
0.01 UTI
0.63
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.01
Cdup
Stellar density (N50/rad) 61.4 [N/pc2]
  • CN 0.63 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.01 Very likely duplicate

Overview

â„šī¸
HSC 1428 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large 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) 194 along with HSC_1427.

Palma et al. (2025)
Part of multiple system G93, along with Gulliver_22, HSC_1427 and HSC_1441.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 84.849 26.354 1.36 -1.525 -4.686 3.44
Hunt & Reffert 2024 84.812 26.348 1.341 -1.55 -4.691 8.985
Hunt & Reffert 2023 84.812 26.348 1.341 -1.55 -4.691 8.985

💡 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– 0.87 0.48 1.48 14 – 117 – –
Liu et al. 2025 1.01 0.25 – 19 – – – –
Hunt & Reffert 2024 – – – – – 117(1) – –
Hunt & Reffert 2023 0.73 0.71 1.48 9 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 22 98.7 84.85 26.36 1.35 -1.52 -4.68 6.62 0.7

💡 Note: The % column shows the percentage of members that HSC 1428 shares with each listed object.

Visualization

â„šī¸