HSC 1614

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0.23 UTI
0.0
CN
0.28
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 15.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.28 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1614 is a sparse, loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, 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.

Close Low extinction Low mass Near-solar metallicity Intermediate age

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 – 101.465 7.939 1.123 -1.265 -3.781 27.35
Zhang et al. 2024 101.478 7.988 – – – –
Hunt & Reffert 2024 101.478 7.988 1.117 -1.186 -3.796 25.915
Cavallo et al. 2024 101.562 7.969 1.12 – – –
Hunt & Reffert 2023 101.478 7.988 1.117 -1.186 -3.796 25.915

💡 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
Zhang et al. 2024 – – – – 0.008* – – –
Hunt & Reffert 2024 – – – – – 42* – –
Cavallo et al. 2024 0.90 0.47 – 275 0.140 – – –
Hunt & Reffert 2023 0.86 0.53 0.64 125 – – – –

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

Visualization

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