HSC 239

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0.31 UTI
0.29
CN
1.0
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 239 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above 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)
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 – 277.989 -7.495 0.4 -0.754 -3.084 -28.55
Hunt & Reffert 2024 277.984 -7.508 0.393 -0.688 -3.034 -14.062
Cavallo et al. 2024 278.017 -7.466 0.394 – – –
Hunt & Reffert 2023 277.984 -7.508 0.393 -0.688 -3.034 -14.062

💡 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 – – – – – 438* – –
Cavallo et al. 2024 2.61 3.84 – 30 0.470 – – –
Hunt & Reffert 2023 2.41 4.30 3.13 84 – – – –

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

Visualization

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