HSC 1410

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0.20 UTI
0.0
CN
0.23
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.23 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1410 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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.

Distant Moderate extinction 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 – 91.4 32.609 0.274 0.857 -1.714 12.07
Zhang et al. 2024 91.359 32.607 – – – –
Hunt & Reffert 2024 91.359 32.607 0.28 0.858 -1.726 –
Cavallo et al. 2024 91.383 32.602 0.28 – – –
Hunt & Reffert 2023 91.359 32.607 0.28 0.858 -1.726 –

💡 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 – – – – -0.244* – – –
Hunt & Reffert 2024 – – – – – 209* – –
Cavallo et al. 2024 3.31 2.15 – 115 -0.520 – – –
Hunt & Reffert 2023 3.48 0.88 1.12 1396 – – – –

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

Visualization

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