CWWDL 14545

0.03 UTI

0.3

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.07

C_dup

C3 classification AA

Number of members (P>50%) 30

Radius (P>50% members) 9.3 [arcmin]

C_N 0.3 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.07 Very likely duplicate

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

Overview

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CWWDL 14545 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below 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 14545 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	–	51.33	30.954	3.373	8.082	-8.19	9.624
Chi et al.	2023	51.386	30.981	3.383	8.116	-8.206	49.693

💡 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	–	–	–	1	0.020	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 1333	93.3	52.28	31.27	3.38	7.39	-9.29	10.82	0.75
HSC 1250	33.3	52.44	31.08	3.39	7.54	-8.24	9.46	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14545 shares with each listed object.

Visualization

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