Theia 1408

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0.05 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.07
Cdup
Radius (P>50% members) 13.6 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.07 Very likely duplicate

Overview

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Theia 1408 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.

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 – 91.704 -2.043 1.738 -0.663 -0.24 40.071
Zhang et al. 2024 91.701 -2.042 – – – –
Hunt & Reffert 2024 91.701 -2.042 1.74 -0.636 -0.283 39.999
Cavallo et al. 2024 91.672 -2.006 1.737 – – –
Hunt & Reffert 2023 91.701 -2.042 1.74 -0.636 -0.283 39.999

💡 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 – – – – -0.088* – – –
Hunt & Reffert 2024 – – – – – 164* – –
Cavallo et al. 2024 0.58 0.62 – 479 0.290 – – –
Hunt & Reffert 2023 0.55 0.26 0.68 735 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 2184 92.9 91.72 -2.04 1.73 -0.66 -0.24 40.14 0.95
CWWDL 14289 39.4 91.68 -2.01 1.74 -0.66 -0.24 40.11 0.0

💡 Note: The % column shows the percentage of members that Theia 1408 shares with each listed object.

Visualization

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