CWWDL 2544

0.05 UTI

0.45

C_N

0.9

C_dens

0.75

C_C3

0.0

C_lit

0.11

C_dup

C3 classification BA

Number of members (P>50%) 45

Radius (P>50% members) 2.8 [arcmin]

C_N 0.45 Poorly populated
C_dens 0.9 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.11 Likely duplicate

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

Overview

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CWWDL 2544 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Metal-poor Young

Data

🔍 Search references for CWWDL 2544 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	–	337.062	59.103	0.258	-3.294	-2.38	87.836
Chi et al.	2023	336.801	58.986	0.266	-3.214	-2.361	-22.12

💡 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	–	–	–	47	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Berkeley 95	88.9	337.07	59.13	0.26	-3.34	-2.37	34.0	0.97
OC 0182	60.0	337.07	59.13	0.26	-3.34	-2.39	87.84	0.0
OC 0183	22.2	337.08	59.14	0.28	-3.33	-2.38	87.84	0.0

💡 Note: The % column shows the percentage of members that CWWDL 2544 shares with each listed object.

Visualization

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