CWWDL 14384

0.26 UTI

0.6

C_N

0.84

C_dens

0.75

C_C3

0.0

C_lit

0.59

C_dup

C3 classification AB

Number of members (P>50%) 69

Radius (P>50% members) 12.2 [arcmin]

C_N 0.6 Moderately populated
C_dens 0.84 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.59 Likely unique

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

Overview

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CWWDL 14384 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a metal-poor, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate 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 14384 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	–	135.757	-46.733	0.874	-6.109	4.01	12.217
Chi et al.	2023	135.744	-46.725	0.884	-6.102	4.01	15.042

💡 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	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1858	100.0	135.75	-46.73	0.87	-6.09	3.99	8.7	0.16
OC 0496	40.6	135.71	-46.74	0.87	-6.08	4.02	26.5	0.28
CWNU 188	36.2	135.69	-46.73	0.88	-6.11	4.01	26.5	0.04

💡 Note: The % column shows the percentage of members that CWWDL 14384 shares with each listed object.

Visualization

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