HSC 2713

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0.32 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2713 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close 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 – 233.151 -55.561 0.458 -0.589 -0.623 –
Hunt & Reffert 2024 233.156 -55.562 0.449 -0.578 -0.631 –
Cavallo et al. 2024 233.186 -55.541 0.45 – – –
Hunt & Reffert 2023 233.156 -55.562 0.449 -0.578 -0.631 –

💡 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 – – – – – 242* – –
Cavallo et al. 2024 1.77 4.67 – 33 -0.300 – – –
Hunt & Reffert 2023 2.12 4.49 1.75 12 – – – –

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

Visualization

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