HSC 2284

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0.14 UTI
0.28
CN
0.15
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.15 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2284 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very large* distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~10.93 kpc) differs significantly from the median photometric distance (~7.31 kpc).

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 Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 147.919 -57.307 0.091 -4.603 3.598 –
Hunt & Reffert 2024 147.887 -57.312 0.091 -4.608 3.572 –
Cavallo et al. 2024 147.978 -57.314 0.099 – – –
Hunt & Reffert 2023 147.887 -57.312 0.091 -4.608 3.572 –

💡 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 – – – – – 698* – –
Cavallo et al. 2024 6.43 3.22 – 81 0.160 – – –
Hunt & Reffert 2023 8.20 4.06 2.36 122 – – – –

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

Visualization

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