Alessi 190

(UBC 5)

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0.80 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad) 18.7 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.62 Moderately studied
  • Cdup 1.0 Unique

Overview

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Alessi 190 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is moderately studied in the literature.

Note: This object shares a significant 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– 238.654 -47.69 1.762 -6.637 -4.167 -18.699
Li et al. 2025 238.548 -47.74 1.785 -6.695 -4.225 –
Alfonso et al. 2024 238.622 -47.68 1.729 -6.618 -4.13 –
Hunt & Reffert 2024 238.748 -47.619 1.754 -6.632 -4.152 -17.938
Cavallo et al. 2024 238.603 -47.702 1.756 – – –
Hunt & Reffert 2023 238.748 -47.619 1.754 -6.632 -4.152 -17.938
He et al. 2022 238.711 -47.634 1.756 -6.633 -4.144 –
Tarricq et al. 2022 238.674 -47.684 1.762 -6.618 -4.13 –
Cantat-Gaudin et al. 2020 238.548 -47.74 1.785 -6.695 -4.225 –
Cantat-Gaudin & Anders 2020 238.548 -47.74 1.785 -6.695 -4.225 –
Bica et al. 2019 238.428 -47.735 – – – –
Castro-Ginard et al. 2018 238.429 -47.729 1.788 -6.699 -4.184 -14.91

💡 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– 0.55 0.835 1.64 209 0.037 229 – –
Li et al. 2025 0.58 0.90 – 450 0.037 – – –
Alfonso et al. 2024 0.55 0.26 – 216 0.010 – – –
Hunt & Reffert 2024 – – – – – 229(1) – –
Cavallo et al. 2024 0.56 1.02 – 257 0.230 – – –
Hunt & Reffert 2023 0.53 0.77 1.64 175 – – – –
He et al. 2022 – 1.20 – 79 – – – –
Tarricq et al. 2022 0.54 – – 209 – – – –
Cantat-Gaudin et al. 2020 0.55 0.26 – 200 – – – –
Cantat-Gaudin & Anders 2020 0.55 – – – – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14469 53.8 238.6 -47.7 1.76 -6.64 -4.14 -18.75 0.0

💡 Note: The % column shows the percentage of members that Alessi 190 shares with each listed object.

Visualization

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