CWNU 2613

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0.31 UTI
0.0
CN
0.32
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.32 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2613 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity Very 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 – 327.776 56.394 0.451 -4.316 -3.642 –
Hunt & Reffert 2024 327.791 56.367 0.459 -4.326 -3.638 5.907
Cavallo et al. 2024 327.71 56.412 0.46 – – –
Hunt & Reffert 2023 327.791 56.367 0.459 -4.326 -3.638 5.907
He et al. 2023 327.716 56.406 0.46 -4.331 -3.642 –

💡 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 – – – – – 487* – –
Cavallo et al. 2024 2.38 2.89 – 7 0.250 – – –
Hunt & Reffert 2023 2.08 3.18 2.04 15 – – – –
He et al. 2023 2.14 3.35 – 8 – – – –

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

Visualization

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