OCSN 41

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0.49 UTI
0.75
CN
0.72
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 45.4 [arcmin]
  • CN 0.75 Rich
  • Cdens 0.72 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

OCSN 41 is a rich, moderately dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 1.44 54.559 2.487 8.277 -4.082 -11.577
Cavallo et al. 2024 1.223 54.433 2.47
Hunt & Reffert 2023 1.078 54.29 2.467 8.212 -4.155 -17.126
Qin et al. 2023 1.07 54.32 2.5 8.34 -4.05 -11.46

💡 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 0.40 0.66 6 -0.040
Hunt & Reffert 2023 0.39 0.08 0.24 7
Qin et al. 2023 0.41 0.28 16

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.