OC 0353

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0.45 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0353 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Close Low 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 – 98.566 -0.878 1.267 -4.147 -0.59 28.936
Zhang et al. 2024 98.563 -0.896 – – – –
Hunt & Reffert 2024 98.563 -0.896 1.247 -4.122 -0.622 26.852
Cavallo et al. 2024 98.575 -0.841 1.254 – – –
Hunt & Reffert 2023 98.563 -0.896 1.247 -4.122 -0.622 26.852
Hao et al. 2022 98.567 -0.895 1.268 -4.135 -0.69 –

💡 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 – – – – -0.440* – – –
Hunt & Reffert 2024 – – – – – 64* – –
Cavallo et al. 2024 0.78 0.41 – 155 0.160 – – –
Hunt & Reffert 2023 0.74 0.20 0.38 189 – – – –
Hao et al. 2022 – 1.27 – 63 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 238 100.0 98.57 -0.88 1.26 -4.15 -0.58 28.77 0.07

💡 Note: The % column shows the percentage of members that OC 0353 shares with each listed object.

Visualization

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