CWWDL 5475

0.00 UTI

0.47

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 47

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

C_N 0.47 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 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 5475 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 5475 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	–	198.218	-64.265	0.459	-4.354	-0.522	-18.401
Chi et al.	2023	198.196	-64.259	0.447	-4.399	-0.497	-25.611

💡 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	–	–	–	76	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 3164	100.0	198.23	-64.26	0.46	-4.34	-0.54	-18.4	0.49
UBC 1522	100.0	198.22	-64.26	0.46	-4.35	-0.53	-18.4	0.02
CWNU 278	51.1	198.22	-64.26	0.45	-4.35	-0.53	-15.14	0.0

💡 Note: The % column shows the percentage of members that CWWDL 5475 shares with each listed object.

Visualization

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