CWNU 2049

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0.28 UTI
0.28
CN
0.65
Cdens
0.38
CC3
0.25
Clit
0.79
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.79 Very likely unique

Overview

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CWNU 2049 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 61.975 53.078 0.306 -0.344 -0.455 -48.271
Hunt & Reffert 2024 61.973 53.106 0.3 -0.334 -0.45 -48.272
Cavallo et al. 2024 61.971 53.085 0.299 – – –
Hunt & Reffert 2023 61.973 53.106 0.3 -0.334 -0.45 -48.272
He et al. 2023 61.964 53.107 0.308 -0.341 -0.452 -48.27

💡 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
Hunt & Reffert 2024 – – – – – 262* – –
Cavallo et al. 2024 3.10 2.33 – 389 0.320 – – –
Hunt & Reffert 2023 3.50 2.43 1.07 191 – – – –
He et al. 2023 3.02 2.45 – 447 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 0408+53 21.4 62.04 53.11 0.3 -0.63 -0.35 – 0.06

💡 Note: The % column shows the percentage of members that CWNU 2049 shares with each listed object.

Visualization

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