CWWDL 6155

0.05 UTI

0.0

C_N

0.08

C_dens

0.38

C_C3

0.0

C_lit

0.6

C_dup

C3 classification BC

Number of members (P>50%) 18

Radius (P>50% members) 8.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.38 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 6155 is a sparse, very loose object of 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 6155 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	–	23.231	60.634	0.339	-1.256	-0.614	–
Chi et al.	2023	23.105	60.39	0.338	-1.226	-0.637	–

💡 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	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 581	40.0	23.34	60.66	0.36	-1.4	-0.58	-38.14	0.96
Gulliver 16	24.0	23.42	60.75	0.21	-1.28	-0.65	-37.02	0.46
Schoenball 1	24.0	23.42	60.75	0.23	-1.29	-0.65	-37.74	0.16

💡 Note: The % column shows the percentage of members that CWWDL 6155 shares with each listed object.

Visualization

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