UBC 1026

Click to load Aladin Lite
0.65 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 1026 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close High extinction Massive Metal-rich 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 – 278.376 -10.715 0.481 0.374 -1.491 -25.519
Hunt & Reffert 2024 278.366 -10.726 0.478 0.355 -1.502 -40.08
Cavallo et al. 2024 278.376 -10.712 0.48 – – –
Hunt & Reffert 2023 278.366 -10.726 0.478 0.355 -1.502 -40.08
Castro-Ginard et al. 2022 278.37 -10.73 0.49 0.38 -1.5 –

💡 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 – – – – – 2063* – –
Cavallo et al. 2024 1.95 4.34 – 76 0.630 – – –
Hunt & Reffert 2023 1.89 4.83 2.46 39 – – – –
Castro-Ginard et al. 2022 2.25 3.94 – 35 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 400 91.9 278.38 -10.72 0.48 0.37 -1.49 -25.52 0.01
CWWDL 1730 51.4 278.37 -10.72 0.49 0.38 -1.49 -26.59 0.0

💡 Note: The % column shows the percentage of members that UBC 1026 shares with each listed object.

Visualization

â„šī¸