OC 0084

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0.00 UTI
0.55
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.55 Moderately 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 0084 is a moderately populated, 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, 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)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 294.037 20.557 0.351 -1.158 -3.96 32.346
Hunt & Reffert 2024 294.028 20.552 0.371 -1.167 -3.967 41.214
Cavallo et al. 2024 294.044 20.56 0.368 – – –
Hunt & Reffert 2023 294.028 20.552 0.371 -1.167 -3.967 41.214
Hao et al. 2022 294.026 20.553 0.347 -1.139 -3.969 27.448

💡 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 – – – – – 1930* – –
Cavallo et al. 2024 2.82 4.14 – 93 0.470 – – –
Hunt & Reffert 2023 2.55 4.25 2.80 103 – – – –
Hao et al. 2022 – 1.80 – 158 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 313 100.0 294.04 20.56 0.35 -1.17 -3.95 32.28 0.55

💡 Note: The % column shows the percentage of members that OC 0084 shares with each listed object.

Visualization

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