OC 0428

Click to load Aladin Lite
0.00 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
OC 0428 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied 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.

Distant Moderate 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 – 117.646 -29.951 0.318 -2.748 3.438 –
Hunt & Reffert 2024 117.637 -29.947 0.307 -2.741 3.423 –
Cavallo et al. 2024 117.641 -29.943 0.309 – – –
Hunt & Reffert 2023 117.637 -29.947 0.307 -2.741 3.423 –
Hao et al. 2022 117.632 -29.942 0.329 -2.733 3.447 –

💡 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 – – – – – 472* – –
Cavallo et al. 2024 3.58 2.52 – 50 0.510 – – –
Hunt & Reffert 2023 2.87 2.24 0.72 66 – – – –
Hao et al. 2022 – 1.42 – 32 0.323 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 236 100.0 117.64 -29.95 0.31 -2.74 3.45 – 0.46

💡 Note: The % column shows the percentage of members that OC 0428 shares with each listed object.

Visualization

â„šī¸