Theia 2448

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0.03 UTI
0.0
CN
0.32
Cdens
0.75
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 6.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.32 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

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Theia 2448 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close 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 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 Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 151.801 -59.74 0.511 -5.209 5.41 27.712
Hunt & Reffert 2024 151.926 -59.729 0.512 -5.226 5.43 31.409
Cavallo et al. 2024 151.799 -59.782 0.518 – – –
Hunt & Reffert 2023 151.926 -59.729 0.512 -5.226 5.43 31.409

💡 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 – – – – – 111* – –
Cavallo et al. 2024 1.64 0.25 – 355 0.150 – – –
Hunt & Reffert 2023 1.79 0.20 0.59 302 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
PHOC 12 84.0 151.73 -59.72 0.51 -5.21 5.41 – 0.21

💡 Note: The % column shows the percentage of members that Theia 2448 shares with each listed object.

Visualization

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