HSC 714

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0.07 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 714 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very 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 distant High extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 318.544 48.673 0.138 -2.998 -3.232 -57.609
Hunt & Reffert 2024 318.565 48.643 0.139 -3.0 -3.229 -33.749
Cavallo et al. 2024 318.558 48.682 0.137 – – –
Hunt & Reffert 2023 318.565 48.643 0.139 -3.0 -3.229 -33.749

💡 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 – – – – – 1159* – –
Cavallo et al. 2024 4.00 4.11 – 19 0.170 – – –
Hunt & Reffert 2023 7.50 4.36 2.39 9 – – – –

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

Visualization

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