CWNU 1107

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0.51 UTI
0.31
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1107 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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.
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 – 329.735 63.988 0.99 -3.119 -4.213 -29.39
Hunt & Reffert 2024 329.745 63.985 1.011 -3.183 -4.228 -19.087
Cavallo et al. 2024 329.606 63.904 1.011 – – –
Hunt & Reffert 2023 329.745 63.985 1.011 -3.183 -4.228 -19.087
He et al. 2022 329.764 63.972 0.99 -3.103 -4.149 –

💡 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 – – – – – 118* – –
Cavallo et al. 2024 1.10 1.53 – 4 -0.290 – – –
Hunt & Reffert 2023 0.97 1.38 1.83 7 – – – –
He et al. 2022 – 1.35 – 6 – – – –

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

Visualization

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