CWWDL 14127

0.13 UTI

0.41

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.29

C_dup

C3 classification AB

Number of members (P>50%) 41

Radius (P>50% members) 6.7 [arcmin]

C_N 0.41 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.29 Possibly duplicate

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

Overview

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CWWDL 14127 is a poorly populated, very dense object of high 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 14127 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	–	126.968	-42.723	0.69	-5.681	4.788	19.756
Chi et al.	2023	126.921	-42.714	0.69	-5.486	4.774	39.898

💡 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	–	–	–	4	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
PHOC 1	70.7	127.0	-42.77	0.69	-5.71	4.8	19.76	0.5
HSC 2091	9.8	126.73	-42.64	0.67	-5.08	4.67	13.84	0.37

💡 Note: The % column shows the percentage of members that CWWDL 14127 shares with each listed object.

Visualization

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