OC 0689

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0.02 UTI
0.58
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.03
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.03 Very likely duplicate

Overview

â„šī¸
OC 0689 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age 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 Intermediate age

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 – 263.513 -35.064 0.503 -0.189 -2.282 -12.456
Hunt & Reffert 2024 263.526 -35.065 0.501 -0.187 -2.293 -7.023
Cavallo et al. 2024 263.519 -35.05 0.499 – – –
Hunt & Reffert 2023 263.526 -35.065 0.501 -0.187 -2.293 -7.023
Hao et al. 2022 263.496 -35.059 0.522 -0.191 -2.238 –

💡 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 – – – – – 1888* – –
Cavallo et al. 2024 1.58 4.64 – 123 -0.400 – – –
Hunt & Reffert 2023 1.87 4.23 2.46 100 – – – –
Hao et al. 2022 – 3.77 – 100 0.051 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2106 97.0 263.5 -35.06 0.49 -0.21 -2.26 -14.34 0.55

💡 Note: The % column shows the percentage of members that OC 0689 shares with each listed object.

Visualization

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