Alessi J0622.4+2114

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0.54 UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 14.2 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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Alessi J0622.4+2114 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 95.591 21.244 0.301 -0.313 -0.124 31.482
Zhang et al. 2024 95.593 21.249 – – – –
Hunt & Reffert 2024 95.593 21.249 0.297 -0.31 -0.127 31.483
Cavallo et al. 2024 95.581 21.248 0.296 – – –
Hunt & Reffert 2023 95.593 21.249 0.297 -0.31 -0.127 31.483
Bica et al. 2019 95.606 21.249 – – – –

💡 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– 3.18 1.445 0.75 332 -0.239 194 – –
Zhang et al. 2024 – – – – -0.249(1) – – –
Hunt & Reffert 2024 – – – – – 194(1) – –
Cavallo et al. 2024 3.39 1.70 – 282 -0.230 – – –
Hunt & Reffert 2023 2.97 1.19 0.75 381 – – – –

(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 1404 100.0 95.59 21.24 0.3 -0.31 -0.13 31.48 0.02

💡 Note: The % column shows the percentage of members that Alessi J0622.4+2114 shares with each listed object.

Visualization

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