OC 0356

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0.42 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.76
Cdup
Radius (P>50% members) 16.3 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.76 Very likely unique

Overview

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OC 0356 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

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

Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 85.301 -9.475 2.254 0.562 -1.278 15.986
Cavallo et al. 2024 85.291 -9.564 2.219 – – –
Hunt & Reffert 2023 85.286 -9.524 2.217 0.549 -1.481 52.254
Hao et al. 2022 85.272 -9.388 2.255 0.511 -1.229 22.144

💡 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
Cavallo et al. 2024 0.79 2.86 – 13 0.250 – – –
Hunt & Reffert 2023 0.43 2.24 1.01 5 – – – –
Hao et al. 2022 – 1.15 – 2 0.323 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 70 100.0 85.34 -9.45 2.27 0.53 -1.21 16.14 0.32
FSR 1088 24.3 85.27 -9.35 2.29 0.49 -1.2 16.61 0.47
Cmg 109 4.7 85.25 -8.97 2.22 0.48 -1.0 16.48 0.45

💡 Note: The % column shows the percentage of members that OC 0356 shares with each listed object.

Visualization

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