Theia 2649

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0.01 UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.02
Cdup
Radius (P>50% members) 10.2 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.02 Very likely duplicate

Overview

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Theia 2649 is a moderately populated, very dense object of 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 – 106.85 -7.665 0.924 -3.942 1.206 32.252
Hunt & Reffert 2024 106.884 -7.665 0.911 -3.935 1.184 31.628
Cavallo et al. 2024 106.798 -7.651 0.919 – – –
Hunt & Reffert 2023 106.884 -7.665 0.911 -3.935 1.184 31.628

💡 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 – – – – – 166* – –
Cavallo et al. 2024 1.12 0.40 – 85 0.430 – – –
Hunt & Reffert 2023 1.02 0.18 0.47 133 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
PHOC 4 98.3 106.82 -7.65 0.92 -3.94 1.18 33.55 0.46
HXHWL 54 93.2 106.85 -7.66 0.93 -3.94 1.21 32.38 0.0
CMa01 88.1 106.81 -7.67 0.93 -3.93 1.19 32.25 0.0

💡 Note: The % column shows the percentage of members that Theia 2649 shares with each listed object.

Visualization

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