CWNU 2871

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0.01 UTI
0.52
CN
1.0
Cdens
0.5
CC3
0.25
Clit
0.02
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.02 Very likely duplicate

Overview

â„šī¸
CWNU 2871 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction Massive Metal-rich Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 316.071 50.22 0.333 -4.087 -5.221 48.352
Hunt & Reffert 2024 316.067 50.225 0.337 -4.087 -5.169 65.685
Cavallo et al. 2024 316.113 50.206 0.338 – – –
Hunt & Reffert 2023 316.067 50.225 0.337 -4.087 -5.169 65.685
He et al. 2023 316.086 50.209 0.342 -4.067 -5.228 –

💡 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 – – – – – 1216* – –
Cavallo et al. 2024 3.87 4.84 – 16 0.630 – – –
Hunt & Reffert 2023 2.60 5.14 2.95 41 – – – –
He et al. 2023 3.39 6.00 – 1 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0292 98.1 316.07 50.22 0.35 -4.08 -5.19 100.55 0.48

💡 Note: The % column shows the percentage of members that CWNU 2871 shares with each listed object.

Visualization

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