Alessi 116

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0.66 UTI
0.7
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 15.1 [arcmin]
  • CN 0.7 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Alessi 116 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

Cavallo et al. (2024)
Gold 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– 310.213 20.163 1.076 -6.286 -9.296 24.381
Hu & Soubiran 2025 310.159 20.191 – – – –
Hunt & Reffert 2024 310.244 20.07 1.067 -6.267 -9.232 23.622
Cavallo et al. 2024 310.159 20.191 1.077 – – –
Hunt & Reffert 2023 310.244 20.07 1.067 -6.267 -9.232 23.622
Bica et al. 2019 310.292 20.065 – – – –

💡 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– 0.875 0.315 0.45 1036 -0.200 136 – –
Hu & Soubiran 2025 – – – – -0.200(5) – – –
Hunt & Reffert 2024 – – – – – 136(1) – –
Cavallo et al. 2024 0.87 0.50 – 977 -0.200 – – –
Hunt & Reffert 2023 0.88 0.13 0.45 1094 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UPK 84 100.0 310.22 20.21 1.08 -6.29 -9.29 24.19 0.3
CWWDL 14281 61.1 310.2 20.17 1.07 -6.28 -9.3 23.99 0.0
UBC 131 34.4 310.18 20.07 1.06 -6.26 -9.29 24.32 0.0

💡 Note: The % column shows the percentage of members that Alessi 116 shares with each listed object.

Visualization

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