CWWDL 14618

0.00 UTI

0.26

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification DA

Number of members (P>50%) 26

Radius (P>50% members) 12.9 [arcmin]

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 14618 is a poorly populated, very dense object of intermediate 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 14618 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	–	298.492	26.208	1.833	2.356	-2.213	-12.477
Chi et al.	2023	298.572	26.117	1.843	2.385	-2.23	-16.61

💡 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	–	–	–	7	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2417	100.0	298.32	26.4	1.83	2.32	-2.16	-16.28	0.0
UPK 82	100.0	298.35	26.41	1.84	2.3	-2.15	-17.01	0.87

💡 Note: The % column shows the percentage of members that CWWDL 14618 shares with each listed object.

Visualization

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