CWWDL 5648

0.00 UTI

0.72

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 94

Radius (P>50% members) 3.8 [arcmin]

C_N 0.72 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high 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 5648 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, 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 Young

Data

🔍 Search references for CWWDL 5648 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	–	236.583	-56.801	0.381	-1.68	-3.219	-43.576
Chi et al.	2023	236.579	-56.805	0.379	-1.702	-3.22	-0.75

💡 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	–	–	–	66	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1180	100.0	236.58	-56.8	0.38	-1.68	-3.22	-45.53	0.0
UBC 306	100.0	236.57	-56.8	0.37	-1.69	-3.22	-43.62	0.12
UFMG 1	100.0	236.58	-56.8	0.37	-1.67	-3.23	-43.98	0.69
OC 0633	38.3	236.59	-56.8	0.38	-1.67	-3.2	99.63	0.0

💡 Note: The % column shows the percentage of members that CWWDL 5648 shares with each listed object.

Visualization

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