HSC 1708

Click to load Aladin Lite
0.24 UTI
0.0
CN
0.46
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.46 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1708 is a sparse, loose object of high C3 quality. Its parallax locates it at a very large distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 100.82 -4.855 0.087 0.127 0.337 –
Hunt & Reffert 2024 100.825 -4.856 0.096 0.127 0.315 –
Hunt & Reffert 2023 100.825 -4.856 0.096 0.127 0.315 –

💡 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– 9.61 1.59 1.18 124 – 423 – –
Hunt & Reffert 2024 – – – – – 423(1) – –
Hunt & Reffert 2023 9.61 1.59 1.18 124 – – – –

(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 3116 80.0 100.82 -4.85 0.09 0.09 0.34 95.85 0.05

💡 Note: The % column shows the percentage of members that HSC 1708 shares with each listed object.

Visualization

â„šī¸