OC 0644

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0.00 UTI
0.25
CN
1.0
Cdens
0.5
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
OC 0644 is a poorly populated, very dense object of intermediate 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 – 241.557 -52.136 0.373 -2.863 -4.82 -36.026
Hunt & Reffert 2024 241.566 -52.134 0.372 -2.864 -4.801 -5.408
Cavallo et al. 2024 241.578 -52.14 0.373 – – –
Hunt & Reffert 2023 241.566 -52.134 0.372 -2.864 -4.801 -5.408
Hao et al. 2022 241.562 -52.132 0.41 -2.916 -4.807 –

💡 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 – – – – – 1523* – –
Cavallo et al. 2024 2.45 3.77 – 148 0.500 – – –
Hunt & Reffert 2023 2.46 3.82 2.62 98 – – – –
Hao et al. 2022 – 0.00 – 63 0.370 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1614 100.0 241.57 -52.13 0.37 -2.85 -4.8 -34.47 0.55

💡 Note: The % column shows the percentage of members that OC 0644 shares with each listed object.

Visualization

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