OCSN 65

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0.57 UTI
0.81
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.82
Cdup
Radius (P>50% members) 32.1 [arcmin]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 0.82 Very likely unique

Overview

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OCSN 65 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 low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported 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, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Very close Low extinction Near-solar metallicity Very young

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 – 83.789 -1.805 2.366 -1.311 0.921 27.08
Zhang et al. 2024 83.764 -2.155 – – – –
Hunt & Reffert 2024 83.764 -2.155 2.365 -1.258 0.93 33.161
Cavallo et al. 2024 83.749 -1.836 2.362 – – –
Hunt & Reffert 2023 83.764 -2.155 2.365 -1.258 0.93 33.161
Qin et al. 2023 83.88 -1.79 2.37 -1.34 0.93 26.34

💡 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 – – – – -0.133* – – –
Hunt & Reffert 2024 – – – – – 52* – –
Cavallo et al. 2024 0.44 0.85 – 5 -0.190 – – –
Hunt & Reffert 2023 0.41 0.36 0.58 13 – – – –
Qin et al. 2023 0.52 0.59 – 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 6 17.6 83.34 -1.63 2.41 -0.07 -0.24 28.06 0.68
OCSN 194 14.5 83.32 -1.64 2.42 -0.06 -0.25 28.06 0.02
OCSN 61 0.4 84.06 -0.59 2.56 -1.03 -0.63 29.9 0.51

💡 Note: The % column shows the percentage of members that OCSN 65 shares with each listed object.

Visualization

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