CWNU 155

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0.61 UTI
0.56
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 155 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 273.451 -21.061 0.777 0.829 -0.946 -7.244
Hunt & Reffert 2024 273.462 -21.062 0.769 0.839 -0.923 19.64
Cavallo et al. 2024 273.468 -21.066 0.771 – – –
Hunt & Reffert 2023 273.462 -21.062 0.769 0.839 -0.923 19.64
He et al. 2022 273.452 -21.08 0.78 0.81 -0.95 –

💡 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 – – – – – 357* – –
Cavallo et al. 2024 1.36 1.40 – 18 -0.600 – – –
Hunt & Reffert 2023 1.21 0.95 1.09 14 – – – –
He et al. 2022 1.58 1.14 – 10 0.744 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14149 47.6 273.45 -21.07 0.78 0.8 -0.93 -24.18 0.0

💡 Note: The % column shows the percentage of members that CWNU 155 shares with each listed object.

Visualization

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