OCSN 59

Click to load Aladin Lite
0.51 UTI
0.55
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 24.6 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OCSN 59 is a moderately populated, 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 object shares a large percentage of members with a later reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

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

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 77.141 -3.206 2.584 1.213 -0.943 22.683
Cavallo et al. 2024 77.27 -2.948 2.586 – – –
Hunt & Reffert 2023 76.844 -3.336 2.584 1.197 -0.859 17.392
Qin et al. 2023 77.03 -3.25 2.61 1.26 -0.8 15.41

💡 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 0.39 0.90 – 11 0.160 – – –
Hunt & Reffert 2023 0.38 0.45 1.30 6 – – – –
Qin et al. 2023 0.43 0.31 – 8 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
LISC-III 3613 91.5 77.17 -3.08 2.59 1.22 -0.8 24.1 0.14

💡 Note: The % column shows the percentage of members that OCSN 59 shares with each listed object.

Visualization

â„šī¸