Theia 11

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0.48 UTI
0.34
CN
1.0
Cdens
1.0
CC3
0.03
Clit
1.0
Cdup
Core radius and density 0.8 [pc], 5.7 [pc-2]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 11 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P87, along with Collinder_471.

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.49 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.49 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 341.517 75.134 2.905 7.387 0.292 -16.689
Cavallo et al. 2024 341.089 75.238 2.915 – – –
Hunt & Reffert 2023 341.328 75.155 2.913 7.332 0.521 -44.971
Kounkel & Covey 2019 341.373 75.182 2.79 – – -5.477

💡 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] Bfrac BSS
UCC 99999– 0.36 0.8 1.77 6 0.170 – – –
Cavallo et al. 2024 0.39 1.85 – 6 0.170 – – –
Hunt & Reffert 2023 0.33 0.49 1.77 5 – – – –
Kounkel & Covey 2019 0.36 0.80 – 6 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
LDN 1251 100.0 340.96 75.2 2.9 7.34 0.48 -34.04 0.43
OC 0209 79.4 341.35 75.11 2.91 7.34 0.29 -16.69 0.03
OCSN 39 76.5 340.59 75.18 2.9 7.07 0.65 -48.18 0.0

💡 Note: The % column shows the percentage of members that Theia 11 shares with each listed object.

Visualization

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