OC 0175

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0.00 UTI
0.45
CN
1.0
Cdens
0.25
CC3
0.31
Clit
0.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
OC 0175 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate 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 – 334.716 57.436 0.321 -4.391 -3.587 -72.644
Hu & Soubiran 2025 334.736 57.435 – – – –
Hunt & Reffert 2024 334.722 57.435 0.313 -4.383 -3.565 -72.641
Cavallo et al. 2024 334.736 57.435 0.314 – – –
Hunt & Reffert 2023 334.722 57.435 0.313 -4.383 -3.565 -72.641
Hao et al. 2022 334.752 57.43 0.325 -4.409 -3.561 -75.146

💡 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
Hu & Soubiran 2025 – – – – -0.150* – – –
Hunt & Reffert 2024 – – – – – 780* – –
Cavallo et al. 2024 2.43 2.76 – 676 0.060 – – –
Hunt & Reffert 2023 2.88 2.84 1.95 288 – – – –
Hao et al. 2022 – 3.62 – 631 0.274 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2547 100.0 334.72 57.43 0.32 -4.4 -3.57 -66.8 0.03
FoF 1809 100.0 334.71 57.43 0.32 -4.4 -3.55 -60.96 0.42

💡 Note: The % column shows the percentage of members that OC 0175 shares with each listed object.

Visualization

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