HSC 2325

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0.28 UTI
0.49
CN
0.16
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2325 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Distant Very high extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 154.515 -57.342 0.172 -5.516 3.39 18.801
Hunt & Reffert 2024 154.588 -57.327 0.163 -5.529 3.405 31.4
Cavallo et al. 2024 154.323 -57.294 0.162 – – –
Hunt & Reffert 2023 154.588 -57.327 0.163 -5.529 3.405 31.4

💡 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 – – – – – 1982* – –
Cavallo et al. 2024 3.61 5.00 – 45 0.220 – – –
Hunt & Reffert 2023 5.48 5.42 2.98 43 – – – –

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

Visualization

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