CWNU 1136

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0.35 UTI
0.59
CN
0.39
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 187.9 [arcmin]
  • CN 0.59 Moderately populated
  • Cdens 0.39 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

CWNU 1136 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 4 later reported entries. See table with shared members information.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 186.943 -60.634 9.216 -36.687 -12.148 12.268
He et al. 2022 187.592 -59.435 9.213 -36.298 -12.088

💡 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
He et al. 2022 0.05 14

💡 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.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 177 88.2 185.96 -63.25 9.36 -37.38 -11.21 12.41 0.44
OCSN 178 64.7 191.21 -57.65 8.99 -34.71 -14.46 11.89 0.47
HSC 2468 57.4 185.31 -56.63 9.04 -35.54 -11.74 12.65 0.24
HSC 2505 36.8 185.58 -64.05 9.33 -37.8 -10.73 12.41 0.0

💡 Note: The % column shows the percentage of members that CWNU 1136 shares with each listed object.

Visualization

Galactocentric position diagram

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