HSC 2798

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0.33 UTI
0.42
CN
0.17
Cdens
1.0
CC3
0.03
Clit
1.0
Cdup
Core radius and density 2.3 [pc], 0.8 [pc-2]
  • CN 0.42 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2798 is a poorly populated, very loose object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, 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 optical pair P488, along with HSC_2794.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.09 (50th percentile), true positive? (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.09 (50th percentile), true positive? (human-assigned).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 248.81 -46.169 0.219 -2.732 -3.391 -82.894
Hunt & Reffert 2024 248.809 -46.18 0.218 -2.719 -3.364 –
Cavallo et al. 2024 248.801 -46.17 0.218 – – –
Hunt & Reffert 2023 248.809 -46.18 0.218 -2.719 -3.364 –

💡 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– 3.88 4.68 2.665 39 -0.210 2636 – –
Hunt & Reffert 2024 3.88 4.68 2.66 39 – 2636(1) – –
Cavallo et al. 2024 3.34 4.68 – 18 -0.210 – – –
Hunt & Reffert 2023 3.88 4.68 2.67 39 – – – –

(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 4040 88.1 248.82 -46.15 0.23 -2.73 -3.42 – 0.14

💡 Note: The % column shows the percentage of members that HSC 2798 shares with each listed object.

Visualization

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