HSC 839

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0.38 UTI
0.33
CN
0.32
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.32 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 839 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Distant Moderate 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 – 344.378 56.829 0.302 -3.631 -2.761 -75.679
Zhang et al. 2024 344.385 56.82 – – – –
Hunt & Reffert 2024 344.385 56.82 0.306 -3.65 -2.753 -75.705
Cavallo et al. 2024 344.287 56.855 0.306 – – –
Hunt & Reffert 2023 344.385 56.82 0.306 -3.65 -2.753 -75.705

💡 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
Zhang et al. 2024 – – – – -0.117* – – –
Hunt & Reffert 2024 – – – – – 322* – –
Cavallo et al. 2024 3.52 1.49 – 100 0.700 – – –
Hunt & Reffert 2023 3.08 1.72 1.44 26 – – – –

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

Visualization

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