CWNU 2149

0.41 UTI

0.25

C_N

0.9

C_dens

0.25

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 25

Radius (P>50% members) 3.0 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.9 Very dense
C_C3 0.25 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 2149 is a poorly populated, very dense object of low 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Relatively close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 2149 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	325.266	55.067	0.371	-5.7	-5.161	-56.225
Hu & Soubiran	2025	325.257	55.063	–	–	–	–
Hunt & Reffert	2024	325.261	55.083	0.365	-5.69	-5.171	-56.174
Cavallo et al.	2024	325.257	55.063	0.366	–	–	–
Hunt & Reffert	2023	325.261	55.083	0.365	-5.69	-5.171	-56.174
He et al.	2023	325.291	55.041	0.381	-5.686	-5.151	–

💡 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
Hu & Soubiran	2025	–	–	–	–	-0.130*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	315*	–	–
Cavallo et al.	2024	2.78	3.72	–	851	0.440	–	–	–
Hunt & Reffert	2023	2.31	4.08	2.56	367	–	–	–	–
He et al.	2023	2.34	3.70	–	1413	–	–	–	–

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

Visualization

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