HSC 2408

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0.11 UTI
0.62
CN
1.0
Cdens
0.5
CC3
0.0
Clit
0.27
Cdup
Radius (P>50% members) 39.9 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.27 Possibly duplicate

Overview

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HSC 2408 is a moderately populated, very dense object of intermediate 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, intermediate-age 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 Intermediate age

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 – 169.403 -58.977 3.764 -23.529 6.114 12.605
Cavallo et al. 2024 166.793 -58.555 3.668 – – –
Hunt & Reffert 2023 169.508 -59.086 3.646 -22.521 6.732 10.976

💡 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 0.28 0.64 – 89 0.220 – – –
Hunt & Reffert 2023 0.26 0.14 0.44 128 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1139 73.0 169.49 -59.06 3.78 -23.75 6.05 12.61 0.41

💡 Note: The % column shows the percentage of members that HSC 2408 shares with each listed object.

Visualization

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