CWWDL 12546

0.00 UTI

0.29

C_N

0.6

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BB

Number of members (P>50%) 29

Radius (P>50% members) 3.2 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.6 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 12546 is a poorly populated, moderately dense object of intermediate 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 12546 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	–	107.347	0.531	0.3	-1.004	-0.674	59.45
Chi et al.	2023	107.353	0.518	0.323	-0.999	-0.624	–

💡 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	–	–	–	35	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1344	100.0	107.35	0.54	0.28	-1.01	-0.68	59.45	0.5
CWNU 192	82.8	107.35	0.53	0.3	-1.02	-0.68	–	0.0
CWWDL 12541	69.0	107.35	0.53	0.28	-1.0	-0.66	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 12546 shares with each listed object.

Visualization

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