HSC 1914

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0.10 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1914 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

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.

Very distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 113.044 -24.706 0.137 -0.772 1.39 87.426
Hunt & Reffert 2024 113.06 -24.729 0.12 -0.803 1.388 94.263
Cavallo et al. 2024 113.013 -24.719 0.121 – – –
Hunt & Reffert 2023 113.06 -24.729 0.12 -0.803 1.388 94.263

💡 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 – – – – – 369* – –
Cavallo et al. 2024 4.33 2.28 – 234 -0.320 – – –
Hunt & Reffert 2023 7.77 2.78 1.72 40 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4148 92.0 113.03 -24.7 0.14 -0.77 1.41 73.6 0.12

💡 Note: The % column shows the percentage of members that HSC 1914 shares with each listed object.

Visualization

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