OC 0675

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0.56 UTI
0.3
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0675 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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.

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 – 260.778 -44.381 0.876 2.096 -3.255 -20.113
Hunt & Reffert 2024 260.77 -44.378 0.826 2.222 -3.059 -3.344
Cavallo et al. 2024 260.73 -44.265 0.831 – – –
Hunt & Reffert 2023 260.77 -44.378 0.826 2.222 -3.059 -3.344
Hao et al. 2022 260.777 -44.386 0.898 2.11 -3.278 –

💡 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 – – – – – 476* – –
Cavallo et al. 2024 1.06 0.90 – 59 0.320 – – –
Hunt & Reffert 2023 1.12 0.95 1.61 21 – – – –
Hao et al. 2022 – 4.30 – 50 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 316 100.0 260.78 -44.37 0.88 2.09 -3.28 -20.11 0.12
CWWDL 14110 100.0 260.79 -44.39 0.88 2.1 -3.26 -20.11 0.0

💡 Note: The % column shows the percentage of members that OC 0675 shares with each listed object.

Visualization

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