CWWDL 14110

0.00 UTI

0.35

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 35

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

C_N 0.35 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high 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 14110 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a metal-poor, very 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. See table with shared members information.

Metal-poor Very young

Data

🔍 Search references for CWWDL 14110 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	–	260.786	-44.388	0.877	2.095	-3.261	-20.113
Chi et al.	2023	260.786	-44.385	0.885	2.118	-3.243	-18.465

💡 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	–	–	–	2	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 316	100.0	260.78	-44.37	0.88	2.09	-3.28	-20.11	0.12
OC 0675	85.7	260.78	-44.38	0.88	2.1	-3.25	-20.11	0.56

💡 Note: The % column shows the percentage of members that CWWDL 14110 shares with each listed object.

Visualization

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