Theia 1907

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0.09 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.2
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.2 Likely duplicate

Overview

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Theia 1907 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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 Moderate 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 – 245.07 -44.886 0.763 0.46 -2.263 -37.705
Hunt & Reffert 2024 245.066 -44.878 0.764 0.468 -2.252 -59.824
Cavallo et al. 2024 245.07 -45.059 0.766 – – –
Hunt & Reffert 2023 245.066 -44.878 0.764 0.468 -2.252 -59.824

💡 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 – – – – – 223* – –
Cavallo et al. 2024 1.25 1.59 – 138 0.210 – – –
Hunt & Reffert 2023 1.23 1.33 1.45 164 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 16 80.0 245.07 -44.87 0.76 0.48 -2.27 -37.71 0.45

💡 Note: The % column shows the percentage of members that Theia 1907 shares with each listed object.

Visualization

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