CWWDL 14154

0.01 UTI

0.58

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.02

C_dup

C3 classification AA

Number of members (P>50%) 66

Radius (P>50% members) 8.9 [arcmin]

C_N 0.58 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

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

Overview

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CWWDL 14154 is a moderately populated, very dense object of very 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 14154 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	–	87.456	27.022	1.055	-0.328	-1.0	-3.588
Chi et al.	2023	87.455	26.983	1.066	-0.328	-0.977	1.748

💡 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	–	–	–	6	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
COIN-Gaia 23	98.5	87.45	27.03	1.05	-0.33	-1.01	-0.01	0.14
Majaess 65	87.9	87.45	27.04	1.04	-0.33	-1.01	-0.05	0.69
Alessi 135	37.9	87.41	27.04	1.05	-0.34	-1.03	-3.7	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14154 shares with each listed object.

Visualization

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