Theia 1884

Click to load Aladin Lite
0.31 UTI
0.25
CN
0.95
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.95 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1884 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, below 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.
Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 125.311 -42.431 0.62 -6.12 4.932 –
Cavallo et al. 2024 125.674 -42.864 0.592 – – –
Hunt & Reffert 2023 125.293 -42.414 0.594 -6.122 4.891 –

💡 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
Cavallo et al. 2024 1.70 1.68 – 34 0.250 – – –
Hunt & Reffert 2023 1.60 1.42 1.90 31 – – – –

Visualization

â„šī¸