HSC 80

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0.13 UTI
0.0
CN
0.3
Cdens
0.5
CC3
0.0
Clit
0.84
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.84 Very likely unique

Overview

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HSC 80 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~2.85 kpc) differs significantly from the median photometric distance (~2.05 kpc).

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

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Metal-poor 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 – 270.254 -24.328 0.351 0.118 -1.468 17.568
Hunt & Reffert 2024 270.255 -24.335 0.34 0.107 -1.473 16.276
Cavallo et al. 2024 270.254 -24.334 0.34 – – –
Hunt & Reffert 2023 270.255 -24.335 0.34 0.107 -1.473 16.276

💡 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 – – – – – 597* – –
Cavallo et al. 2024 1.43 4.13 – 81 -0.690 – – –
Hunt & Reffert 2023 2.67 3.84 2.61 12 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 596 16.0 270.22 -24.23 0.39 0.06 -1.42 25.14 0.22

💡 Note: The % column shows the percentage of members that HSC 80 shares with each listed object.

Visualization

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