HSC 2931

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0.28 UTI
0.29
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.62
Cdup
Radius (P>50% members) 43.0 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.62 Likely unique

Overview

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HSC 2931 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by moderate 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 Moderate 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 – 245.13 -21.677 7.406 -11.332 -25.067 -5.207
Cavallo et al. 2024 245.074 -21.824 7.447 – – –
Hunt & Reffert 2023 245.127 -21.673 7.447 -11.444 -25.056 -4.234

💡 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 0.13 1.58 – 8 -0.260 – – –
Hunt & Reffert 2023 0.13 0.51 0.52 6 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 245 37.9 246.4 -24.04 7.2 -7.05 -25.65 -7.74 0.53

💡 Note: The % column shows the percentage of members that HSC 2931 shares with each listed object.

Visualization

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