Theia 2510

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0.00 UTI
0.45
CN
0.8
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 10.0 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.8 Dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 2510 is a poorly populated, dense object of very high 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 – 277.012 -15.363 0.868 -2.662 -3.569 12.939
Hunt & Reffert 2024 277.04 -15.331 0.859 -2.622 -3.549 12.506
Cavallo et al. 2024 277.008 -15.382 0.863 – – –
Hunt & Reffert 2023 277.04 -15.331 0.859 -2.622 -3.549 12.506

💡 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 – – – – – 208* – –
Cavallo et al. 2024 1.00 0.92 – 309 -0.180 – – –
Hunt & Reffert 2023 1.10 0.74 0.38 159 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 57 100.0 276.99 -15.35 0.87 -2.67 -3.57 12.94 0.18
CWWDL 14359 86.7 277.01 -15.36 0.87 -2.67 -3.59 16.41 0.02
PHOC 20 71.1 277.0 -15.39 0.87 -2.67 -3.59 16.41 0.43

💡 Note: The % column shows the percentage of members that Theia 2510 shares with each listed object.

Visualization

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