Theia 711

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0.04 UTI
0.0
CN
0.3
Cdens
0.38
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 30.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

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Theia 711 is a sparse, loose object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Very close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 282.208 -7.559 2.296 1.128 -11.4 -10.747
Hunt & Reffert 2024 282.094 -7.744 2.305 1.065 -11.383 -9.119
Cavallo et al. 2024 281.992 -7.4 2.299 – – –
Hunt & Reffert 2023 282.094 -7.744 2.305 1.065 -11.383 -9.119

💡 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 – – – – – 53* – –
Cavallo et al. 2024 0.45 1.43 – 30 -0.030 – – –
Hunt & Reffert 2023 0.41 0.85 1.92 62 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 7 68.0 282.41 -7.21 2.3 1.14 -11.29 -7.59 0.09

💡 Note: The % column shows the percentage of members that Theia 711 shares with each listed object.

Visualization

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