CWNU 1243

0.33 UTI

0.38

C_N

0.54

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 38

Stellar density (N₅₀/rad) 2.7 [N/pc²]

C3 classification DB

C_N 0.38 Poorly populated
C_dens 0.54 Moderately dense
C_C3 0.25 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 1243 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Close Low extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for CWNU 1243 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	99999–	307.84	39.013	1.051	-1.001	-4.42	-9.735
Zhang et al.	2024	307.955	39.043	–	–	–	–
Cavallo et al.	2024	307.846	38.994	1.061	–	–	–
Hunt & Reffert	2023	307.955	39.043	1.065	-0.983	-4.403	-0.466
He et al.	2022	307.889	39.023	1.066	-1.044	-4.406	–

💡 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]	B_frac	BSS
UCC	99999–	0.975	0.96	0.57	13	-0.013	–	–	–
Zhang et al.	2024	–	–	–	–	-0.165⁽¹⁾	–	–	–
Cavallo et al.	2024	1.04	0.96	–	12	0.140	–	–	–
Hunt & Reffert	2023	0.91	0.83	0.57	13	–	–	–	–
He et al.	2022	–	1.90	–	25	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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