HSC 2789

Click to load Aladin Lite
0.17 UTI
0.0
CN
0.61
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.61 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2789 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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.

Close Low 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 – 247.255 -46.104 1.121 -0.968 -2.992 12.426
Hunt & Reffert 2024 247.237 -46.121 1.112 -0.995 -2.952 -19.973
Cavallo et al. 2024 247.332 -46.064 1.114 – – –
Hunt & Reffert 2023 247.237 -46.121 1.112 -0.995 -2.952 -19.973

💡 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 – – – – – 65* – –
Cavallo et al. 2024 0.76 0.73 – 170 0.190 – – –
Hunt & Reffert 2023 0.85 0.80 0.57 87 – – – –

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

Visualization

â„šī¸