HSC 2137

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0.08 UTI
0.0
CN
0.14
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 13.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2137 is a sparse, very loose object of 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 near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Near-solar metallicity Intermediate age

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 – 133.7 -44.445 0.675 -4.286 1.765 10.063
Hunt & Reffert 2024 133.615 -44.438 0.681 -4.275 1.811 10.115
Cavallo et al. 2024 133.825 -44.439 0.677 – – –
Hunt & Reffert 2023 133.615 -44.438 0.681 -4.275 1.811 10.115

💡 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 – – – – – 101* – –
Cavallo et al. 2024 1.73 3.78 – 74 0.300 – – –
Hunt & Reffert 2023 1.41 3.25 2.40 418 – – – –

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

Visualization

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