HSC 1481

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0.23 UTI
0.26
CN
0.15
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 94.7 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.15 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1481 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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.

Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 76.359 19.446 4.742 -0.6 -8.436 9.678
Zhang et al. 2024 78.451 15.828 – – – –
Cavallo et al. 2024 77.632 18.481 4.716 – – –
Hunt & Reffert 2023 78.451 15.828 4.733 -0.689 -8.264 19.244

💡 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 – – – – 0.076* – – –
Cavallo et al. 2024 0.21 1.13 – 16 0.020 – – –
Hunt & Reffert 2023 0.22 0.54 0.72 26 – – – –

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

Visualization

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