CWWDL 14639

0.06 UTI

0.47

C_N

0.14

C_dens

0.75

C_C3

0.0

C_lit

0.21

C_dup

N_m (P>50%) 47

Core radius and density 2.5 [pc], 0.7 [pc^-2]

C3 classification BA

C_N 0.47 Poorly populated
C_dens 0.14 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14639 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a 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 likely a duplicate object, which shares a large 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 14639 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	99999–	112.41	-12.371	1.876	-5.828	-1.023	16.023
Chi et al.	2023	112.263	-12.278	1.885	-5.864	-1.058	15.692

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	8	0.120	–	–	–
Chi et al.	2023	–	–	–	8	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2424	78.7	112.51	-12.56	1.88	-5.81	-0.99	17.56	0.26
OCSN 77	76.6	112.55	-12.52	1.87	-5.82	-1.0	17.56	0.04

💡 Note: The % column shows the percentage of members that CWWDL 14639 shares with each listed object.

Visualization

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