OC 0149

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0.50 UTI
0.49
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0149 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high 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 a later reported entry. See table with shared members information.

Relatively close High extinction Near-solar metallicity 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 – 316.707 53.01 0.556 -2.3 -2.241 -13.624
Hunt & Reffert 2024 316.716 53.021 0.549 -2.297 -2.213 -13.603
Cavallo et al. 2024 316.717 53.015 0.553 – – –
Hunt & Reffert 2023 316.716 53.021 0.549 -2.297 -2.213 -13.603
Hao et al. 2022 316.722 53.012 0.56 -2.275 -2.235 –

💡 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 – – – – – 506* – –
Cavallo et al. 2024 2.57 4.19 – 23 0.580 – – –
Hunt & Reffert 2023 1.69 4.10 2.83 64 – – – –
Hao et al. 2022 – 3.05 – 1 0.051 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 253 93.9 316.71 53.02 0.55 -2.31 -2.23 -13.62 0.09

💡 Note: The % column shows the percentage of members that OC 0149 shares with each listed object.

Visualization

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