HSC 836

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0.15 UTI
0.26
CN
0.13
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.7 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 836 is a poorly populated, very loose object of low 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant High extinction Near-solar metallicity Intermediate age

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 – 341.449 59.302 0.264 -2.836 -2.123 36.433
Hunt & Reffert 2024 341.429 59.304 0.282 -2.883 -2.104 –
Cavallo et al. 2024 341.458 59.291 0.28 – – –
Hunt & Reffert 2023 341.429 59.304 0.282 -2.883 -2.104 –

💡 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 – – – – – 593* – –
Cavallo et al. 2024 3.15 3.17 – 275 -0.100 – – –
Hunt & Reffert 2023 3.45 3.81 2.56 23 – – – –

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

Visualization

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