HSC 1093

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0.28 UTI
0.0
CN
0.33
Cdens
1.0
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.4 [pc], 1.7 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.33 Loose
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1093 is a sparse, loose object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the age parameter (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.

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– 39.832 64.618 0.135 -1.379 0.495 –
Hunt & Reffert 2024 39.826 64.619 0.13 -1.385 0.496 –
Cavallo et al. 2024 39.844 64.619 0.135 – – –
Hunt & Reffert 2023 39.826 64.619 0.13 -1.385 0.496 –

💡 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– 6.08 2.59 0.6 24 -0.860 365 – –
Hunt & Reffert 2024 6.08 2.59 0.60 24 – 365(1) – –
Cavallo et al. 2024 2.99 2.90 – 151 -0.860 – – –
Hunt & Reffert 2023 6.08 2.59 0.60 24 – – – –

(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 3168 100.0 39.85 64.62 0.12 -1.39 0.5 – 0.08

💡 Note: The % column shows the percentage of members that HSC 1093 shares with each listed object.

Visualization

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