Theia 2901

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0.02 UTI
0.31
CN
0.42
Cdens
0.5
CC3
0.25
Clit
0.06
Cdup
Radius (P>50% members) 11.1 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.42 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.06 Very likely duplicate

Overview

â„šī¸
Theia 2901 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near 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 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 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 – 75.819 42.109 0.844 1.022 -3.425 -19.179
Zhang et al. 2024 75.835 42.089 – – – –
Hunt & Reffert 2024 75.835 42.089 0.842 1.061 -3.415 -18.534
Cavallo et al. 2024 75.831 42.097 0.844 – – –
Hunt & Reffert 2023 75.835 42.089 0.842 1.061 -3.415 -18.534

💡 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
Zhang et al. 2024 – – – – -0.082* – – –
Hunt & Reffert 2024 – – – – – 140* – –
Cavallo et al. 2024 1.16 0.55 – 316 0.200 – – –
Hunt & Reffert 2023 1.11 0.36 0.53 225 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1098 93.5 75.82 42.11 0.84 1.02 -3.42 -17.96 0.28

💡 Note: The % column shows the percentage of members that Theia 2901 shares with each listed object.

Visualization

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