OC 0367

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0.50 UTI
0.25
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.25 Poorly 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 0367 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Close Low extinction Near-solar metallicity Very young

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 – 89.462 -14.103 1.48 -2.043 1.628 28.575
Hunt & Reffert 2024 89.451 -14.114 1.488 -1.867 1.52 27.353
Cavallo et al. 2024 89.577 -14.164 1.488 – – –
Hunt & Reffert 2023 89.451 -14.114 1.488 -1.867 1.52 27.353
Hao et al. 2022 89.432 -14.1 1.48 -1.953 1.698 27.735

💡 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 – – – – – 75* – –
Cavallo et al. 2024 0.75 1.00 – 5 -0.130 – – –
Hunt & Reffert 2023 0.64 0.47 1.58 7 – – – –
Hao et al. 2022 – 1.13 – 4 0.498 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14262 92.0 89.46 -14.1 1.49 -2.03 1.58 26.55 0.14
CWNU 18 72.0 89.47 -14.09 1.5 -2.01 1.64 26.55 0.11

💡 Note: The % column shows the percentage of members that OC 0367 shares with each listed object.

Visualization

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