CWWDL 6027

0.02 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.0

C_lit

0.6

C_dup

C3 classification DC

Number of members (P>50%) 16

Radius (P>50% members) 8.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.6 Likely unique

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

Overview

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CWWDL 6027 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, very 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 Very young

Data

🔍 Search references for CWWDL 6027 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	–	335.195	54.922	0.245	-3.72	-3.045	-19.764
Chi et al.	2023	335.261	54.954	0.249	-3.766	-3.07	–

💡 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	–	–	–	1	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 1369	40.0	335.15	54.99	0.26	-3.82	-3.13	-84.73	0.03
OC 0169	4.0	334.44	55.0	0.31	-3.64	-3.12	-41.54	0.14

💡 Note: The % column shows the percentage of members that CWWDL 6027 shares with each listed object.

Visualization

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