HSC 845

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0.13 UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 845 is a sparse, very loose object of intermediate 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, very young 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 Very 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 – 343.183 59.157 0.331 -3.321 -2.741 -69.923
Hunt & Reffert 2024 343.186 59.157 0.328 -3.327 -2.732 -13.728
Cavallo et al. 2024 343.198 59.182 0.324 – – –
Hunt & Reffert 2023 343.186 59.157 0.328 -3.327 -2.732 -13.728

💡 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 – – – – – 259* – –
Cavallo et al. 2024 3.84 4.33 – 15 -0.260 – – –
Hunt & Reffert 2023 2.99 3.42 1.78 20 – – – –

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

Visualization

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