CWNU 2555

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0.55 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.5 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 2555 is a moderately populated, very dense object of high 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.
Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 334.121 55.514 0.203 -3.054 -2.784 -96.421
Hunt & Reffert 2024 334.123 55.512 0.201 -3.074 -2.78 -98.435
Cavallo et al. 2024 334.109 55.519 0.204 – – –
Hunt & Reffert 2023 334.123 55.512 0.201 -3.074 -2.78 -98.435
He et al. 2023 334.115 55.512 0.216 -3.054 -2.784 -102.84

💡 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 – – – – – 697* – –
Cavallo et al. 2024 4.29 2.55 – 692 -0.390 – – –
Hunt & Reffert 2023 4.25 2.49 1.99 374 – – – –
He et al. 2023 5.01 2.60 – 1259 – – – –

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

Visualization

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