OC 0619

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0.00 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.0 Sparse
  • 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 0619 is a sparse, 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, 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.

Relatively close High extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 223.9 -60.52 0.313 -5.178 -3.337 47.792
Hunt & Reffert 2024 223.877 -60.52 0.306 -5.187 -3.334 33.366
Cavallo et al. 2024 223.91 -60.522 0.306 – – –
Hunt & Reffert 2023 223.877 -60.52 0.306 -5.187 -3.334 33.366
Hao et al. 2022 223.939 -60.509 0.317 -5.185 -3.344 –

💡 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 – – – – – 1591* – –
Cavallo et al. 2024 2.62 4.47 – 49 0.170 – – –
Hunt & Reffert 2023 2.90 4.36 2.38 41 – – – –
Hao et al. 2022 – 2.76 – 5 0.169 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1175 100.0 223.89 -60.52 0.3 -5.18 -3.33 31.71 0.48

💡 Note: The % column shows the percentage of members that OC 0619 shares with each listed object.

Visualization

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