HSC 849

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0.12 UTI
0.3
CN
0.12
Cdens
0.25
CC3
0.0
Clit
0.9
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.12 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.9 Very likely unique

Overview

â„šī¸
HSC 849 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 moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.9) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Palma et al. (2025)
Classified as optical pair P58, along with King_10.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 344.201 58.788 0.255 -3.395 -2.129 –
Hunt & Reffert 2024 344.215 58.78 0.263 -3.397 -2.153 –
Cavallo et al. 2024 344.251 58.743 0.26 – – –
Hunt & Reffert 2023 344.215 58.78 0.263 -3.397 -2.153 –

💡 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] Bfrac BSS
UCC 99999– 3.51 2.45 2.51 80 0.770 326 – –
Hunt & Reffert 2024 – – – – – 326(1) – –
Cavallo et al. 2024 3.73 2.47 – 102 0.770 – – –
Hunt & Reffert 2023 3.29 2.43 2.51 59 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2155 10.0 344.08 58.56 0.3 -3.51 -2.29 – 0.08

💡 Note: The % column shows the percentage of members that HSC 849 shares with each listed object.

Visualization

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