Theia 3409

Click to load Aladin Lite
0.03 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.07
Cdup
Stellar density (N50/rad) 10.5 [N/pc2]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.07 Very likely duplicate

Overview

â„šī¸
Theia 3409 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low 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 very likely a duplicate object, which shares a large 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– 159.031 -60.646 0.401 -7.722 2.651 -7.446
Hunt & Reffert 2024 159.056 -60.648 0.387 -7.69 2.67 -7.465
Cavallo et al. 2024 159.045 -60.64 0.392 – – –
Hunt & Reffert 2023 159.056 -60.648 0.387 -7.69 2.67 -7.465

💡 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– 2.23 0.44 0.91 156 0.190 635 – –
Hunt & Reffert 2024 – – – – – 635(1) – –
Cavallo et al. 2024 2.17 0.38 – 132 0.190 – – –
Hunt & Reffert 2023 2.29 0.50 0.91 179 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1483 93.1 159.03 -60.64 0.41 -7.72 2.65 -7.45 0.5
CWWDL 5091 61.8 159.03 -60.63 0.41 -7.69 2.64 -7.45 0.04

💡 Note: The % column shows the percentage of members that Theia 3409 shares with each listed object.

Visualization

â„šī¸