HSC 806

Click to load Aladin Lite
0.16 UTI
0.0
CN
0.44
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.44 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 806 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, 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.

Distant High extinction Near-solar metallicity Intermediate age

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 – 333.126 58.285 0.206 -4.59 -2.24 -70.784
Hunt & Reffert 2024 333.132 58.316 0.203 -4.593 -2.195 -64.793
Cavallo et al. 2024 333.134 58.291 0.202 – – –
Hunt & Reffert 2023 333.132 58.316 0.203 -4.593 -2.195 -64.793

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 507* – –
Cavallo et al. 2024 4.53 4.07 – 339 -0.280 – – –
Hunt & Reffert 2023 4.28 3.82 1.91 627 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3587 76.0 333.14 58.29 0.21 -4.64 -2.24 -70.7 0.04

💡 Note: The % column shows the percentage of members that HSC 806 shares with each listed object.

Visualization

â„šī¸