OC 0041

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0.47 UTI
0.35
CN
0.77
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.77 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0041 is a poorly populated, dense object of 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 near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction 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 – 278.304 -7.991 0.52 -0.308 -2.696 81.905
Hunt & Reffert 2024 278.312 -7.986 0.506 -0.31 -2.722 31.703
Cavallo et al. 2024 278.292 -7.987 0.506 – – –
Hunt & Reffert 2023 278.312 -7.986 0.506 -0.31 -2.722 31.703
Hao et al. 2022 278.29 -7.986 0.535 -0.319 -2.659 –

💡 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 – – – – – 592* – –
Cavallo et al. 2024 1.75 3.72 – 240 0.140 – – –
Hunt & Reffert 2023 1.82 3.75 2.24 66 – – – –
Hao et al. 2022 – 3.96 – 398 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 494 100.0 278.32 -7.99 0.5 -0.31 -2.7 40.94 0.36

💡 Note: The % column shows the percentage of members that OC 0041 shares with each listed object.

Visualization

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