HSC 2442

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0.19 UTI
0.58
CN
0.45
Cdens
0.5
CC3
0.0
Clit
0.62
Cdup
Radius (P>50% members) 64.7 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 0.45 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.62 Likely unique

Overview

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HSC 2442 is a moderately populated, loose 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, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Very 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 – 170.957 -71.151 3.49 -21.893 -1.34 4.719
Cavallo et al. 2024 170.407 -70.841 3.525 – – –
Hunt & Reffert 2023 165.239 -70.58 3.52 -21.839 -1.358 -1.207

💡 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 0.30 0.93 – 13 -0.040 – – –
Hunt & Reffert 2023 0.28 0.38 0.79 26 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1196 37.9 168.39 -70.64 3.45 -21.72 -0.65 4.72 0.22

💡 Note: The % column shows the percentage of members that HSC 2442 shares with each listed object.

Visualization

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