CWWDL 14377

0.01 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.01

C_dup

C3 classification AB

Number of members (P>50%) 104

Radius (P>50% members) 11.8 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.01 Very likely duplicate

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

Overview

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CWWDL 14377 is a rich, very dense 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 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14377 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	–	107.264	-7.189	1.136	-0.89	-1.196	1.22
Chi et al.	2023	107.254	-7.156	1.138	-0.862	-1.161	5.243

💡 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	–	–	–	5	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FOF 2302	99.0	107.26	-7.2	1.14	-0.9	-1.2	3.48	0.5
OC 0370	89.4	107.27	-7.19	1.14	-0.89	-1.19	1.12	0.0
Theia 361	20.2	107.27	-7.22	1.17	-0.92	-1.16	6.2	0.01

💡 Note: The % column shows the percentage of members that CWWDL 14377 shares with each listed object.

Visualization

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