Theia 2115

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0.00 UTI
0.41
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 2115 is a poorly populated, very dense 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, young 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 Young

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 – 239.436 -53.067 0.721 -3.277 -3.201 -15.804
Hunt & Reffert 2024 239.435 -53.053 0.729 -3.264 -3.194 -28.113
Cavallo et al. 2024 239.441 -53.061 0.73 – – –
Hunt & Reffert 2023 239.435 -53.053 0.729 -3.264 -3.194 -28.113

💡 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 – – – – – 219* – –
Cavallo et al. 2024 1.41 2.71 – 41 0.320 – – –
Hunt & Reffert 2023 1.29 2.74 1.85 37 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 256 100.0 239.44 -53.07 0.72 -3.28 -3.2 -15.8 0.19
CWWDL 13864 100.0 239.44 -53.07 0.72 -3.28 -3.2 -15.8 0.02
OC 0637 63.4 239.43 -53.06 0.73 -3.28 -3.2 -15.8 0.4

💡 Note: The % column shows the percentage of members that Theia 2115 shares with each listed object.

Visualization

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