Theia 415

Click to load Aladin Lite
0.10 UTI
0.0
CN
0.14
Cdens
0.38
CC3
0.25
Clit
0.48
Cdup
Radius (P>50% members) 21.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.48 Possibly duplicate

Overview

â„šī¸
Theia 415 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age 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.

Close Low extinction Low mass Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 83.102 38.384 1.168 -0.615 -2.07 -6.456
Zhang et al. 2024 83.133 38.331 – – – –
Hunt & Reffert 2024 83.133 38.331 1.175 -0.63 -2.046 -7.066
Cavallo et al. 2024 83.005 38.413 1.185 – – –
Hunt & Reffert 2023 83.133 38.331 1.175 -0.63 -2.046 -7.066

💡 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 – – – – 0.006* – – –
Hunt & Reffert 2024 – – – – – 48* – –
Cavallo et al. 2024 0.87 0.59 – 126 0.290 – – –
Hunt & Reffert 2023 0.80 0.69 0.40 92 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0288 52.0 82.73 38.48 1.16 -0.76 -2.15 -14.57 0.08

💡 Note: The % column shows the percentage of members that Theia 415 shares with each listed object.

Visualization

â„šī¸