HSC 2468

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0.24 UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.42
Cdup
Radius (P>50% members) 153.4 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.42 Possibly duplicate

Overview

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HSC 2468 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 185.307 -56.626 9.041 -35.542 -11.737 12.649
Cavallo et al. 2024 185.435 -56.158 9.082 – – –
Hunt & Reffert 2023 182.229 -51.54 9.084 -35.27 -11.962 12.903

💡 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
Cavallo et al. 2024 0.11 1.03 – 36 0.090 – – –
Hunt & Reffert 2023 0.11 0.20 0.67 8 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 178 57.5 191.21 -57.65 8.99 -34.71 -14.46 11.89 0.47
OCSN 177 27.8 185.96 -63.25 9.36 -37.38 -11.21 12.41 0.44
CWNU 1136 18.4 186.94 -60.63 9.22 -36.69 -12.15 12.27 0.35
OCSN 176 0.9 183.96 -51.2 8.38 -33.21 -11.16 12.82 0.52

💡 Note: The % column shows the percentage of members that HSC 2468 shares with each listed object.

Visualization

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