CWNU 2675

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0.56 UTI
0.54
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.54 Moderately 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 2675 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 192.665 -64.383 0.442 -4.432 -1.254 -2.667
Hunt & Reffert 2024 192.647 -64.382 0.444 -4.43 -1.26 –
Cavallo et al. 2024 192.643 -64.449 0.442 – – –
Hunt & Reffert 2023 192.647 -64.382 0.444 -4.43 -1.26 –
He et al. 2023 192.642 -64.388 0.443 -4.428 -1.256 –

💡 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 – – – – – 406* – –
Cavallo et al. 2024 2.06 2.13 – 45 -0.440 – – –
Hunt & Reffert 2023 2.11 1.71 2.42 44 – – – –
He et al. 2023 2.19 1.95 – 14 – – – –

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

Visualization

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