HSC 2683

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0.40 UTI
0.25
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2683 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Very high extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 228.442 -58.197 0.328 -4.696 -4.119 75.295
Hunt & Reffert 2024 228.435 -58.186 0.322 -4.687 -4.144 57.685
Cavallo et al. 2024 228.436 -58.191 0.323 – – –
Hunt & Reffert 2023 228.435 -58.186 0.322 -4.687 -4.144 57.685

💡 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 – – – – – 843* – –
Cavallo et al. 2024 2.16 5.48 – 48 0.460 – – –
Hunt & Reffert 2023 2.84 5.89 1.50 10 – – – –

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

Visualization

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