HSC 2095

Click to load Aladin Lite
0.09 UTI
0.0
CN
0.09
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2095 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, below 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.

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)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 127.929 -42.664 0.193 -3.155 3.896 67.062
Hunt & Reffert 2024 127.942 -42.668 0.193 -3.148 3.858 66.236
Cavallo et al. 2024 127.949 -42.693 0.19 – – –
Hunt & Reffert 2023 127.942 -42.668 0.193 -3.148 3.858 66.236

💡 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 – – – – – 603* – –
Cavallo et al. 2024 3.98 3.15 – 191 0.280 – – –
Hunt & Reffert 2023 4.62 3.65 2.31 40 – – – –

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

Visualization

â„šī¸