HSC 2193

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0.40 UTI
0.26
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.7 [arcmin]
  • CN 0.26 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 2193 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close* distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~0.72 kpc) differs significantly from the median photometric distance (~1.11 kpc).

Relatively close High extinction Near-solar metallicity Old

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 – 137.53 -48.675 1.392 -7.626 3.565 8.0
Hunt & Reffert 2024 137.497 -48.686 1.398 -7.625 3.572 21.474
Cavallo et al. 2024 137.51 -48.682 1.419 – – –
Hunt & Reffert 2023 137.497 -48.686 1.398 -7.625 3.572 21.474

💡 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 – – – – – 74* – –
Cavallo et al. 2024 1.53 2.42 – 4169 0.250 – – –
Hunt & Reffert 2023 0.69 3.83 1.75 9 – – – –

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

Visualization

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