CWWDL 574

0.05 UTI

0.52

C_N

0.62

C_dens

0.75

C_C3

0.0

C_lit

0.13

C_dup

C3 classification AB

Number of members (P>50%) 54

Radius (P>50% members) 4.3 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.62 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.13 Likely duplicate

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

Overview

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CWWDL 574 is a moderately populated, moderately dense object of 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 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 574 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	–	335.685	53.731	0.299	-2.836	-2.464	-60.916
Chi et al.	2023	335.659	53.722	0.302	-2.854	-2.455	-60.21

💡 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	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1157	87.0	335.69	53.73	0.3	-2.83	-2.46	-60.92	0.21
LISC 1103	53.7	335.68	53.71	0.3	-2.85	-2.48	-58.26	0.43

💡 Note: The % column shows the percentage of members that CWWDL 574 shares with each listed object.

Visualization

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