OC 0493

Click to load Aladin Lite
0.44 UTI
0.45
CN
0.24
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.24 Very loose
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0493 is a poorly populated, very loose object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Distant Moderate extinction Massive 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 – 131.515 -48.148 0.174 -3.031 3.76 55.66
Hunt & Reffert 2024 131.463 -48.136 0.175 -3.042 3.769 56.826
Cavallo et al. 2024 131.5 -48.132 0.173 – – –
Hunt & Reffert 2023 131.463 -48.136 0.175 -3.042 3.769 56.826
Hao et al. 2022 131.536 -48.163 0.179 -3.051 3.76 –

💡 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 – – – – – 1590* – –
Cavallo et al. 2024 4.29 1.72 – 398 0.290 – – –
Hunt & Reffert 2023 5.16 2.00 1.86 206 – – – –
Hao et al. 2022 – 1.70 – 158 0.537 – – –

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

Visualization

â„šī¸