OCSN 13

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0.33 UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.6
Cdup
Radius (P>50% members) 17.4 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.6 Likely unique

Overview

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OCSN 13 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported 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.

Close Low extinction Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 291.746 21.107 2.002 1.546 -6.639 -10.02
Qin et al. 2023 291.75 21.1 2.0 1.43 -6.47 -10.37

💡 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
Qin et al. 2023 0.59 0.46 – 8 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0083 40.5 291.76 21.1 1.99 1.58 -6.74 -8.47 0.54
OC 0081 23.3 291.8 20.88 2.01 1.65 -6.78 -11.01 0.5
Theia 38 11.9 291.82 21.14 2.02 1.23 -6.4 19.11 0.0

💡 Note: The % column shows the percentage of members that OCSN 13 shares with each listed object.

Visualization

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