CWWDL 10854

0.05 UTI

0.0

C_N

0.03

C_dens

0.38

C_C3

0.0

C_lit

0.64

C_dup

C3 classification BC

Number of members (P>50%) 17

Radius (P>50% members) 9.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

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

Overview

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CWWDL 10854 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above 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, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 10854 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	–	98.779	12.473	0.259	-0.296	-0.567	–
Chi et al.	2023	98.832	12.384	0.255	-0.295	-0.597	72.543

💡 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	–	–	–	18	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWL 2009	36.0	98.86	12.49	0.23	-0.21	-0.5	91.35	0.08
CWWDL 10872	4.0	98.45	12.32	0.22	-0.11	-0.54	15.96	0.05

💡 Note: The % column shows the percentage of members that CWWDL 10854 shares with each listed object.

Visualization

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