Theia 2517

Click to load Aladin Lite
0.13 UTI
0.52
CN
0.31
Cdens
0.75
CC3
0.0
Clit
0.42
Cdup
Radius (P>50% members) 16.1 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.31 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.42 Possibly duplicate

Overview

â„šī¸
Theia 2517 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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.

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 – 262.041 -37.838 0.799 3.195 -1.954 -52.221
Hunt & Reffert 2024 262.066 -37.824 0.804 3.197 -1.949 -38.477
Cavallo et al. 2024 261.892 -37.881 0.809 – – –
Hunt & Reffert 2023 262.066 -37.824 0.804 3.197 -1.949 -38.477

💡 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 – – – – – 101* – –
Cavallo et al. 2024 1.15 1.25 – 204 -0.190 – – –
Hunt & Reffert 2023 1.18 1.01 1.21 57 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 85 58.5 262.04 -37.83 0.81 3.21 -1.93 -59.98 0.37

💡 Note: The % column shows the percentage of members that Theia 2517 shares with each listed object.

Visualization

â„šī¸