UBC 1245

Click to load Aladin Lite
0.52 UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 1245 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Near-solar metallicity 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 – 45.572 56.579 0.399 0.674 -1.011 –
Hunt & Reffert 2024 45.57 56.58 0.398 0.662 -1.03 –
Cavallo et al. 2024 45.545 56.579 0.39 – – –
Hunt & Reffert 2023 45.57 56.58 0.398 0.662 -1.03 –
Castro-Ginard et al. 2022 45.57 56.59 0.4 0.67 -1.0 –

💡 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 – – – – – 372* – –
Cavallo et al. 2024 2.72 3.14 – 45 0.450 – – –
Hunt & Reffert 2023 2.31 3.06 1.25 49 – – – –
Castro-Ginard et al. 2022 2.71 2.37 – 269 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 474 97.1 45.58 56.58 0.39 0.68 -1.01 – 0.03

💡 Note: The % column shows the percentage of members that UBC 1245 shares with each listed object.

Visualization

â„šī¸