OC 0017

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0.23 UTI
0.29
CN
0.41
Cdens
0.38
CC3
0.25
Clit
0.72
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.41 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.72 Likely unique

Overview

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OC 0017 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Massive Near-solar metallicity Intermediate age

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 – 272.004 -19.485 0.324 -0.496 -2.019 7.427
Hunt & Reffert 2024 272.01 -19.488 0.337 -0.491 -1.999 16.796
Cavallo et al. 2024 271.975 -19.458 0.333 – – –
Hunt & Reffert 2023 272.01 -19.488 0.337 -0.491 -1.999 16.796
Hao et al. 2022 271.947 -19.503 0.355 -0.531 -1.958 –

💡 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 – – – – – 1355* – –
Cavallo et al. 2024 2.25 5.13 – 117 -0.770 – – –
Hunt & Reffert 2023 2.72 4.29 2.67 144 – – – –
Hao et al. 2022 – 2.64 – 6310 0.051 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 659 27.6 271.87 -19.45 0.36 -0.51 -2.07 126.48 0.25

💡 Note: The % column shows the percentage of members that OC 0017 shares with each listed object.

Visualization

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