HSC 1935

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0.22 UTI
0.25
CN
0.14
Cdens
0.62
CC3
0.03
Clit
1.0
Cdup
Core radius and density 2.8 [pc], 0.7 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1935 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

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.

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– 116.551 -25.598 0.189 -1.68 3.309 –
Hunt & Reffert 2024 116.554 -25.602 0.191 -1.722 3.318 –
Cavallo et al. 2024 116.553 -25.607 0.193 – – –
Hunt & Reffert 2023 116.554 -25.602 0.191 -1.722 3.318 –

💡 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– 4.65 0.73 0.49 726 -0.190 144 – –
Hunt & Reffert 2024 4.65 0.73 0.49 727 – 144(1) – –
Cavallo et al. 2024 5.04 1.60 – 158 -0.190 – – –
Hunt & Reffert 2023 4.65 0.73 0.49 726 – – – –

(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 4033 100.0 116.54 -25.59 0.18 -1.67 3.29 95.04 0.12

💡 Note: The % column shows the percentage of members that HSC 1935 shares with each listed object.

Visualization

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