HSC 715

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0.08 UTI
0.0
CN
0.17
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 10.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 715 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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.

Relatively close Moderate extinction Near-solar metallicity 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 – 314.42 51.113 0.594 -1.604 -0.96 -29.693
Hunt & Reffert 2024 314.491 51.027 0.589 -1.607 -0.94 -14.92
Cavallo et al. 2024 314.441 51.09 0.594 – – –
Hunt & Reffert 2023 314.491 51.027 0.589 -1.607 -0.94 -14.92

💡 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 – – – – – 97* – –
Cavallo et al. 2024 2.52 2.81 – 20 -0.040 – – –
Hunt & Reffert 2023 1.62 2.67 2.33 179 – – – –

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

Visualization

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