HSC 2384

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0.06 UTI
0.64
CN
0.75
Cdens
1.0
CC3
0.0
Clit
0.13
Cdup
Radius (P>50% members) 28.0 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 0.75 Dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.13 Likely duplicate

Overview

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HSC 2384 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 158.562 -64.221 1.795 -16.854 1.61 -4.115
Hunt & Reffert 2024 159.049 -64.212 1.776 -16.865 1.64 -6.128
Cavallo et al. 2024 158.128 -64.162 1.79 – – –
Hunt & Reffert 2023 159.049 -64.212 1.776 -16.865 1.64 -6.128

💡 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
Hunt & Reffert 2024 – – – – – 130* – –
Cavallo et al. 2024 0.54 0.75 – 107 0.350 – – –
Hunt & Reffert 2023 0.53 0.59 1.11 57 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14602 87.0 158.5 -64.2 1.8 -16.85 1.67 -4.47 0.45
CWWDL 14597 49.4 157.74 -64.28 1.79 -16.85 1.81 -4.27 0.31

💡 Note: The % column shows the percentage of members that HSC 2384 shares with each listed object.

Visualization

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