CWNU 2798

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0.44 UTI
0.76
CN
0.71
Cdens
0.75
CC3
0.0
Clit
0.99
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.76 Rich
  • Cdens 0.71 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.99 Unique

Overview

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CWNU 2798 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high 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 – 274.014 -16.471 0.325 -0.766 -2.546 30.149
He et al. 2023 273.998 -16.447 0.339 -0.793 -2.527 0.7

💡 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. 2023 3.89 6.10 – 1 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1756 3.8 274.02 -16.4 0.31 -0.5 -2.12 14.97 0.41
Ryu 212 0.8 274.21 -16.31 0.33 -0.36 -2.39 -0.92 0.31

💡 Note: The % column shows the percentage of members that CWNU 2798 shares with each listed object.

Visualization

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