CWWDL 2672

0.25 UTI

0.78

C_N

0.96

C_dens

0.75

C_C3

0.0

C_lit

0.5

C_dup

C3 classification AB

Number of members (P>50%) 167

Radius (P>50% members) 5.2 [arcmin]

C_N 0.78 Rich
C_dens 0.96 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.5 Likely unique

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

Overview

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CWWDL 2672 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 2672 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	–	105.574	-1.85	0.256	-0.914	0.841	68.399
Chi et al.	2023	105.579	-1.83	0.263	-0.919	0.728	71.523

💡 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	–	–	–	62	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1702	59.9	105.58	-1.86	0.26	-0.91	0.86	66.13	0.01
FoF 373	50.3	105.58	-1.85	0.25	-0.91	0.85	82.74	0.46
OC 0360	15.0	105.58	-1.86	0.25	-0.9	0.86	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 2672 shares with each listed object.

Visualization

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