XDOCC 02

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0.59 UTI
0.51
CN
0.92
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.51 Moderately populated
  • Cdens 0.92 Very dense
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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XDOCC 02 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (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 Low extinction 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 – 84.063 34.298 0.753 0.268 -2.359 9.721
Zhang et al. 2024 84.033 34.291 – – – –
Hunt & Reffert 2024 84.033 34.291 0.756 0.264 -2.356 4.086
Cavallo et al. 2024 84.065 34.298 0.755 – – –
Hunt & Reffert 2023 84.033 34.291 0.756 0.264 -2.356 4.086
Jaehnig et al. 2021 84.049 34.298 0.801 0.285 -2.295 –

💡 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
Zhang et al. 2024 – – – – -0.344* – – –
Hunt & Reffert 2024 – – – – – 191* – –
Cavallo et al. 2024 1.28 0.85 – 56 -0.390 – – –
Hunt & Reffert 2023 1.25 0.51 0.43 35 – – – –
Piatti et al. 2023 – – – 30 0.240 343 0.45 –
Jaehnig et al. 2021 1.26* 0.57 – 35 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2673 92.3 84.06 34.29 0.75 0.27 -2.36 9.72 0.07

💡 Note: The % column shows the percentage of members that XDOCC 02 shares with each listed object.

Visualization

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