HSC 1230

Click to load Aladin Lite
0.03 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 65.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1230 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate 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.

Very close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 59.6 42.21 1.976 -0.025 -7.604 -2.43
Zhang et al. 2024 59.589 42.194 – – – –
Cavallo et al. 2024 59.685 42.329 1.979 – – –
Hunt & Reffert 2023 59.589 42.194 1.98 -0.082 -7.539 -3.323

💡 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
Zhang et al. 2024 – – – – -0.075* – – –
Cavallo et al. 2024 0.50 1.21 – 269 0.150 – – –
Hunt & Reffert 2023 0.48 1.18 1.27 73 – – – –

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

Visualization

â„šī¸