Alessi 80B

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0.21 UTI
0.62
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.33
Cdup
Stellar density (N50/rad) 5.8 [N/pc2]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.33 Possibly duplicate

Overview

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Alessi 80B is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously 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– 268.109 -38.69 0.81 2.901 -1.766 -17.98
Hunt & Reffert 2024 268.132 -38.671 0.791 2.891 -1.749 -16.556
Cavallo et al. 2024 268.184 -38.753 0.8 – – –
Hunt & Reffert 2023 268.132 -38.671 0.791 2.891 -1.749 -16.556
Bica et al. 2019 268.146 -38.64 – – – –

💡 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– 1.165 0.84 1.23 24 -0.180 461 – –
Hunt & Reffert 2024 – – – – – 461(1) – –
Cavallo et al. 2024 1.17 1.04 – 18 -0.180 – – –
Hunt & Reffert 2023 1.16 0.64 1.23 29 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Sco OB5 66.7 268.11 -38.7 0.82 2.9 -1.81 -14.82 0.55

💡 Note: The % column shows the percentage of members that Alessi 80B shares with each listed object.

Visualization

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