CWWDL 12291

0.10 UTI

0.45

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.27

C_dup

C3 classification CB

Number of members (P>50%) 45

Radius (P>50% members) 2.2 [arcmin]

C_N 0.45 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

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

Overview

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CWWDL 12291 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 12291 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	–	312.292	48.711	0.429	-3.182	-5.419	–
Chi et al.	2023	312.291	48.704	0.423	-3.272	-5.445	–

💡 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
Chi et al.	2023	–	–	–	27	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1124	73.3	312.29	48.71	0.43	-3.18	-5.41	–	0.44

💡 Note: The % column shows the percentage of members that CWWDL 12291 shares with each listed object.

Visualization

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