HSC 2935

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0.19 UTI
0.0
CN
0.51
Cdens
0.5
CC3
0.0
Clit
0.92
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.51 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.92 Very likely unique

Overview

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HSC 2935 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.92) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 262.016 -32.823 0.559 -1.296 -2.498 9.639
Hunt & Reffert 2024 262.016 -32.833 0.563 -1.28 -2.49 20.047
Cavallo et al. 2024 261.967 -32.809 0.565 – – –
Hunt & Reffert 2023 262.016 -32.833 0.563 -1.28 -2.49 20.047

💡 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– 1.605 3.185 2.36 31 -0.400 285 – –
Hunt & Reffert 2024 – – – – – 285(1) – –
Cavallo et al. 2024 1.56 3.06 – 49 -0.400 – – –
Hunt & Reffert 2023 1.65 3.31 2.36 13 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 484 8.0 261.9 -32.72 0.46 -1.23 -2.61 -16.52 0.22

💡 Note: The % column shows the percentage of members that HSC 2935 shares with each listed object.

Visualization

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