CWWDL 10687

0.04 UTI

0.0

C_N

0.05

C_dens

0.25

C_C3

0.0

C_lit

0.68

C_dup

C3 classification CC

Number of members (P>50%) 17

Radius (P>50% members) 8.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.68 Likely unique

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

Overview

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CWWDL 10687 is a sparse, very loose object of low 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.

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 Young

Data

🔍 Search references for CWWDL 10687 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	–	41.863	59.845	0.289	-0.532	-0.107	-55.012
Chi et al.	2023	41.839	59.876	0.318	-0.523	-0.112	-44.507

💡 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	–	–	–	58	0.230	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1957	32.0	41.5	59.74	0.28	-0.51	-0.2	-58.28	0.13

💡 Note: The % column shows the percentage of members that CWWDL 10687 shares with each listed object.

Visualization

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