CWNU 2677

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0.23 UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2677 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close 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 – 108.434 -14.833 0.415 -1.006 0.036 –
Hunt & Reffert 2024 108.415 -14.882 0.423 -1.013 0.031 55.946
Cavallo et al. 2024 108.417 -14.834 0.42 – – –
Hunt & Reffert 2023 108.415 -14.882 0.423 -1.013 0.031 55.946
He et al. 2023 108.421 -14.823 0.431 -1.004 0.027 55.94

💡 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 – – – – – 237* – –
Cavallo et al. 2024 2.16 1.32 – 275 0.110 – – –
Hunt & Reffert 2023 2.15 0.97 0.66 322 – – – –
He et al. 2023 2.14 1.30 – 224 – – – –

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

Visualization

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