Theia 248

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0.30 UTI
0.25
CN
0.24
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.24 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 248 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Palma et al. (2025)
Part of multiple system G239, along with Theia_101, OCSN_28 and OCSN_27.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 324.03 53.3 2.086 8.983 6.471 -14.958
Zhang et al. 2024 324.696 53.669 – – – –
Cavallo et al. 2024 323.937 53.124 2.073 – – –
Hunt & Reffert 2023 324.696 53.669 2.077 8.837 6.29 -16.834
He et al. 2022 323.597 53.179 2.079 8.729 6.471 –

💡 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– 0.475 0.95 1.35 112 0.181 – – –
Zhang et al. 2024 – – – – 0.182(1) – – –
Cavallo et al. 2024 0.49 0.95 – 120 0.180 – – –
Hunt & Reffert 2023 0.46 0.61 1.35 112 – – – –
He et al. 2022 – 1.05 – 63 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 30 96.0 323.81 53.28 2.1 8.91 6.5 -16.6 0.19

💡 Note: The % column shows the percentage of members that Theia 248 shares with each listed object.

Visualization

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