Alessi J0622.4+2114

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0.54 UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 1.6 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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. 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.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 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] Bfr BSS
Zhang et al. 2024 -0.249*
Hunt & Reffert 2024 194*
Cavallo et al. 2024 3.39 1.70 282 -0.230
Hunt & Reffert 2023 2.97 1.19 0.75 381

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value 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

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.