Theia 1079

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0.00 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 1079 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied 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 Very 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 – 124.343 -42.574 0.666 -4.772 5.145 38.629
Hunt & Reffert 2024 124.328 -42.54 0.662 -4.771 5.149 38.65
Cavallo et al. 2024 124.403 -42.597 0.664 – – –
Hunt & Reffert 2023 124.328 -42.54 0.662 -4.771 5.149 38.65
He et al. 2022 124.568 -41.852 1.241 -4.74 10.281 –

💡 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 – – – – – 238* – –
Cavallo et al. 2024 1.53 0.87 – 12 0.230 – – –
Hunt & Reffert 2023 1.39 1.11 1.66 10 – – – –
He et al. 2022 – 0.95 – 112 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 479 100.0 124.36 -42.58 0.66 -4.78 5.13 38.63 0.66
CWWDL 3586 94.0 124.35 -42.57 0.67 -4.77 5.14 38.63 0.0

💡 Note: The % column shows the percentage of members that Theia 1079 shares with each listed object.

Visualization

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