CWWDL 14676

0.12 UTI

0.52

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.26

C_dup

C3 classification BA

Number of members (P>50%) 54

Radius (P>50% members) 28.0 [arcmin]

C_N 0.52 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.26 Possibly duplicate

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

Overview

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CWWDL 14676 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, above 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 possibly a duplicate object, which shares a significant 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 14676 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	–	287.766	56.733	3.081	-2.498	3.626	-23.345
Chi et al.	2023	287.722	56.796	3.063	-2.498	3.659	-20.613

💡 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	–	–	–	8	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
RSG4	74.1	287.75	56.79	3.08	-2.51	3.64	-23.08	0.74

💡 Note: The % column shows the percentage of members that CWWDL 14676 shares with each listed object.

Visualization

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