HSC 2986

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0.07 UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.12
Cdup
Stellar density (N50/rad) 10.8 [N/pc2]
  • CN 0.8 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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HSC 2986 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, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.

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

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 257 along with OCSN_3.

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 99999– 283.033 -36.862 6.6 3.099 -27.515 -2.654
Cavallo et al. 2024 282.061 -36.267 6.684 – – –
Hunt & Reffert 2023 285.317 -36.883 6.694 2.209 -27.556 -3.472

💡 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] Bfrac BSS
UCC 99999– 0.15 0.17 0.72 9 -0.040 – – –
Liu et al. 2025 0.15 0.06 – 12 – – – –
Cavallo et al. 2024 0.15 0.89 – 9 -0.040 – – –
Hunt & Reffert 2023 0.15 0.17 0.72 7 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 322 87.6 281.4 -36.61 6.65 1.58 -27.55 -3.06 0.49
OCSN 324 47.1 285.26 -36.93 6.49 4.34 -27.26 -2.82 0.27
UPK 655 25.8 285.35 -36.93 6.49 4.42 -27.19 -5.14 0.51
CWWDL 14680 19.1 280.7 -35.92 6.73 1.19 -27.63 -1.43 0.0

💡 Note: The % column shows the percentage of members that HSC 2986 shares with each listed object.

Visualization

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