CWWDL 14136

0.04 UTI

0.0

C_N

0.29

C_dens

0.38

C_C3

0.0

C_lit

0.28

C_dup

C3 classification CB

Number of members (P>50%) 21

Radius (P>50% members) 8.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.29 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

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CWWDL 14136 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very 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 Very young

Data

🔍 Search references for CWWDL 14136 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	–	99.158	4.849	0.643	-1.431	0.635	–
Chi et al.	2023	99.075	5.049	0.661	-1.407	0.594	–

💡 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	–	–	–	1	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Collinder 104	72.0	99.19	4.79	0.61	-1.42	0.6	36.18	0.76
Collinder 107	40.0	99.25	4.9	0.61	-1.36	0.65	–	0.45

💡 Note: The % column shows the percentage of members that CWWDL 14136 shares with each listed object.

Visualization

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