Theia 546

Click to load Aladin Lite
0.11 UTI
0.34
CN
0.39
Cdens
0.5
CC3
0.25
Clit
0.32
Cdup
Radius (P>50% members) 27.4 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.32 Possibly duplicate

Overview

â„šī¸
Theia 546 is a poorly populated, loose object of intermediate 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 (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.

Close Low extinction Near-solar metallicity Intermediate age

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 – 110.191 -4.303 1.908 -2.152 -3.689 8.192
Zhang et al. 2024 110.172 -4.38 – – – –
Hunt & Reffert 2024 110.172 -4.38 1.91 -2.136 -3.711 8.379
Cavallo et al. 2024 110.415 -4.091 1.904 – – –
Hunt & Reffert 2023 110.172 -4.38 1.91 -2.136 -3.711 8.379

💡 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 – – – – -0.154* – – –
Hunt & Reffert 2024 – – – – – 77* – –
Cavallo et al. 2024 0.54 0.28 – 100 0.060 – – –
Hunt & Reffert 2023 0.50 0.10 0.67 292 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 100 67.6 110.4 -4.3 1.89 -2.15 -3.63 8.4 0.21

💡 Note: The % column shows the percentage of members that Theia 546 shares with each listed object.

Visualization

â„šī¸