HSC 2185

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0.10 UTI
0.27
CN
0.41
Cdens
0.12
CC3
0.0
Clit
0.59
Cdup
Radius (P>50% members) 7.6 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.41 Loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.59 Likely unique

Overview

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HSC 2185 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, 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.

Relatively close High extinction Metal-rich Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 137.455 -47.763 0.608 -5.118 4.108 57.236
Hunt & Reffert 2024 137.458 -47.817 0.62 -5.179 4.115 32.876
Cavallo et al. 2024 137.387 -47.758 0.618 – – –
Hunt & Reffert 2023 137.458 -47.817 0.62 -5.179 4.115 32.876

💡 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 – – – – – 334* – –
Cavallo et al. 2024 1.96 3.20 – 8 0.730 – – –
Hunt & Reffert 2023 1.54 3.49 2.66 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0505 40.7 137.18 -47.89 0.62 -5.17 3.99 70.74 0.13

💡 Note: The % column shows the percentage of members that HSC 2185 shares with each listed object.

Visualization

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