HSC 2982

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0.45 UTI
0.27
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2982 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 264.821 -29.016 0.373 -0.422 -0.521 10.23
Hunt & Reffert 2024 264.808 -29.009 0.367 -0.408 -0.548 16.28
Cavallo et al. 2024 264.818 -29.013 0.379 – – –
Hunt & Reffert 2023 264.808 -29.009 0.367 -0.408 -0.548 16.28

💡 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 – – – – – 2318* – –
Cavallo et al. 2024 3.45 5.10 – 407 0.400 – – –
Hunt & Reffert 2023 2.28 5.83 2.47 321 – – – –

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

Visualization

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