HSC 2634

Click to load Aladin Lite
0.21 UTI
0.3
CN
0.35
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.35 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2634 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young 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 Young

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 212.103 -62.323 0.303 -4.163 -2.519 -31.222
Hunt & Reffert 2024 212.112 -62.319 0.299 -4.174 -2.533 -16.441
Cavallo et al. 2024 212.071 -62.321 0.295 – – –
Hunt & Reffert 2023 212.112 -62.319 0.299 -4.174 -2.533 -16.441

💡 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 – – – – – 491* – –
Cavallo et al. 2024 3.31 3.51 – 45 0.050 – – –
Hunt & Reffert 2023 3.15 4.08 2.61 54 – – – –

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

Visualization

â„šī¸