HSC 1847

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0.09 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.0
Clit
0.88
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

â„šī¸
HSC 1847 is a sparse, very loose object of low 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 (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a 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=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

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 99999– 109.495 -20.006 0.317 -1.689 3.354 –
Hunt & Reffert 2024 109.49 -20.01 0.312 -1.694 3.359 –
Cavallo et al. 2024 109.504 -19.986 0.312 – – –
Hunt & Reffert 2023 109.49 -20.01 0.312 -1.694 3.359 –

💡 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– 2.985 1.525 1.29 23 0.140 275 – –
Hunt & Reffert 2024 – – – – – 275(1) – –
Cavallo et al. 2024 3.25 1.51 – 15 0.140 – – –
Hunt & Reffert 2023 2.72 1.54 1.29 31 – – – –

(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 3952 92.0 109.5 -19.99 0.31 -1.69 3.34 – 0.02
CWWDL 3813 12.0 109.57 -20.05 0.32 -2.02 3.31 – 0.16

💡 Note: The % column shows the percentage of members that HSC 1847 shares with each listed object.

Visualization

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