OC 0290

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0.35 UTI
0.0
CN
1.0
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0290 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, below 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.

Note: This object shares a large percentage of members with a later 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 – 75.404 30.741 0.579 0.766 -2.972 30.664
Hunt & Reffert 2024 75.435 30.759 0.574 0.791 -2.995 30.602
Cavallo et al. 2024 75.405 30.743 0.573 – – –
Hunt & Reffert 2023 75.435 30.759 0.574 0.791 -2.995 30.602
Hao et al. 2022 75.376 30.739 0.587 0.764 -3.018 –

💡 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 – – – – – 133* – –
Cavallo et al. 2024 2.06 1.95 – 282 0.490 – – –
Hunt & Reffert 2023 1.62 1.63 1.36 511 – – – –
Hao et al. 2022 – 0.98 – 398 0.169 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 344 92.0 75.41 30.75 0.58 0.76 -2.97 24.22 0.04

💡 Note: The % column shows the percentage of members that OC 0290 shares with each listed object.

Visualization

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