OC 0652

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0.57 UTI
0.59
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.1 [arcmin]
  • CN 0.59 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0652 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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 significant percentage of members with 2 later reported entries. See table with shared members information.

Close Low 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 – 246.329 -52.204 1.128 0.397 -3.622 -37.508
Hunt & Reffert 2024 246.381 -52.174 1.123 0.376 -3.62 -31.602
Cavallo et al. 2024 246.357 -52.197 1.128 – – –
Hunt & Reffert 2023 246.381 -52.174 1.123 0.376 -3.62 -31.602
Hao et al. 2022 246.335 -52.156 1.136 0.302 -3.594 -25.435

💡 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 – – – – – 218* – –
Cavallo et al. 2024 0.80 0.23 – 347 -0.110 – – –
Hunt & Reffert 2023 0.84 0.23 0.50 205 – – – –
Hao et al. 2022 – 3.19 – 100 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 1071 67.6 246.32 -52.2 1.13 0.4 -3.63 -38.77 0.0
CWWDL 14355 51.5 246.3 -52.21 1.14 0.39 -3.65 -37.46 0.0

💡 Note: The % column shows the percentage of members that OC 0652 shares with each listed object.

Visualization

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