Theia 3475

Click to load Aladin Lite
0.12 UTI
0.33
CN
0.27
Cdens
0.38
CC3
0.25
Clit
0.39
Cdup
Stellar density (N50/rad) 1.3 [N/pc2]
  • CN 0.33 Poorly populated
  • Cdens 0.27 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.39 Possibly duplicate

Overview

â„šī¸
Theia 3475 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported 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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 93.252 24.106 0.521 0.145 -1.969 664.495
Zhang et al. 2024 93.198 24.112 – – – –
Hunt & Reffert 2024 93.198 24.112 0.516 0.146 -1.996 664.493
Cavallo et al. 2024 93.21 23.9 0.516 – – –
Hunt & Reffert 2023 93.198 24.112 0.516 0.146 -1.996 664.493

💡 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– 1.85 1.525 2.38 164 -0.267 242 – –
Zhang et al. 2024 – – – – -0.193(1) – – –
Hunt & Reffert 2024 – – – – – 242(1) – –
Cavallo et al. 2024 1.86 1.56 – 182 -0.340 – – –
Hunt & Reffert 2023 1.84 1.49 2.38 145 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0307 60.6 93.27 24.0 0.52 0.15 -1.93 – 0.23

💡 Note: The % column shows the percentage of members that Theia 3475 shares with each listed object.

Visualization

â„šī¸