CWWDL 14361

0.33 UTI

0.26

C_N

0.88

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 26

Radius (P>50% members) 7.9 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.88 Dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWWDL 14361 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14361 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	–	278.184	-13.02	0.947	0.623	-3.795	-15.236
Chi et al.	2023	278.192	-13.031	0.954	0.57	-3.78	-9.969

💡 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	–	–	–	29	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1829	92.3	278.19	-13.0	0.95	0.62	-3.79	-16.5	0.01

💡 Note: The % column shows the percentage of members that CWWDL 14361 shares with each listed object.

Visualization

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