Theia 2330

Click to load Aladin Lite
0.02 UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.06
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

â„šī¸
Theia 2330 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (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.

Relatively close Moderate extinction Near-solar metallicity Very young

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 – 3.769 63.555 0.467 -3.211 -1.102 -65.487
Hunt & Reffert 2024 3.771 63.553 0.467 -3.154 -1.088 -73.525
Cavallo et al. 2024 4.256 63.55 0.468 – – –
Hunt & Reffert 2023 3.771 63.553 0.467 -3.154 -1.088 -73.525

💡 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 – – – – – 283* – –
Cavallo et al. 2024 2.09 1.79 – 10 -0.050 – – –
Hunt & Reffert 2023 2.03 1.68 1.60 21 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1201 94.1 3.83 63.56 0.47 -3.22 -1.11 -65.49 0.26
Casado 17 55.9 3.83 63.57 0.47 -3.23 -1.08 -65.49 0.24
CWWDL 10501 38.2 4.33 63.56 0.47 -3.16 -1.1 -81.84 0.09

💡 Note: The % column shows the percentage of members that Theia 2330 shares with each listed object.

Visualization

â„šī¸