Theia 4708

Click to load Aladin Lite
0.00 UTI
0.28
CN
0.48
Cdens
0.5
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 9.7 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.48 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
Theia 4708 is a poorly populated, loose object of intermediate 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 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.

Relatively close Moderate 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 – 316.381 57.198 0.824 -1.976 -5.649 -25.427
Hunt & Reffert 2024 316.408 57.19 0.822 -1.987 -5.627 -17.996
Cavallo et al. 2024 316.355 57.194 0.824 – – –
Hunt & Reffert 2023 316.408 57.19 0.822 -1.987 -5.627 -17.996

💡 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
Hunt & Reffert 2024 – – – – – 128* – –
Cavallo et al. 2024 1.18 2.29 – 123 -0.300 – – –
Hunt & Reffert 2023 1.15 1.80 2.24 205 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 380 100.0 316.37 57.23 0.83 -1.99 -5.66 -22.93 0.38

💡 Note: The % column shows the percentage of members that Theia 4708 shares with each listed object.

Visualization

â„šī¸