HSC 1440

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0.27 UTI
0.0
CN
0.49
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 2.5 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.49 Loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1440 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P11, along with CWNU_2105.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 89.156 27.642 0.655 0.141 -2.299 27.49
Zhang et al. 2024 89.143 27.651 – – – –
Hunt & Reffert 2024 89.143 27.651 0.647 0.131 -2.294 4.741
Cavallo et al. 2024 89.108 27.635 0.652 – – –
Hunt & Reffert 2023 89.143 27.651 0.647 0.131 -2.294 4.741

💡 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– 1.49 0.9 1.44 75 -0.017 133 – –
Zhang et al. 2024 – – – – -0.074(1) – – –
Hunt & Reffert 2024 1.49 0.90 1.44 75 – 133(1) – –
Cavallo et al. 2024 1.58 1.26 – 16 0.040 – – –
Hunt & Reffert 2023 1.49 0.90 1.44 75 – – – –

(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 3789 88.0 89.14 27.64 0.66 0.14 -2.3 27.49 0.03

💡 Note: The % column shows the percentage of members that HSC 1440 shares with each listed object.

Visualization

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