HSC 1445

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0.09 UTI
0.0
CN
0.02
Cdens
0.75
CC3
0.06
Clit
0.52
Cdup
Core radius and density 3.5 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 0.52 Likely unique

Overview

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HSC 1445 is a sparse, very 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (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– 90.288 27.224 0.512 -0.225 -2.291 -33.008
Zhang et al. 2024 90.325 27.212 – – – –
Hunt & Reffert 2024 90.325 27.212 0.51 -0.243 -2.298 –
Cavallo et al. 2024 90.409 27.12 0.509 – – –
Hunt & Reffert 2023 90.325 27.212 0.51 -0.243 -2.298 –

💡 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– 1.81 0.77 1.29 106 -0.096 87 – –
Zhang et al. 2024 – – – – -0.191(1) – – –
Hunt & Reffert 2024 1.81 0.76 1.29 106 – 87(1) – –
Cavallo et al. 2024 1.84 0.84 – 56 0.000 – – –
Hunt & Reffert 2023 1.81 0.77 1.29 106 – – – –

(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 2017 48.0 90.15 27.57 0.53 -0.22 -2.24 9.9 0.21

💡 Note: The % column shows the percentage of members that HSC 1445 shares with each listed object.

Visualization

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