CWWDL 10817

0.11 UTI

0.54

C_N

0.1

C_dens

0.25

C_C3

0.0

C_lit

0.65

C_dup

C3 classification CC

Number of members (P>50%) 57

Radius (P>50% members) 9.9 [arcmin]

C_N 0.54 Moderately populated
C_dens 0.1 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.65 Likely unique

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

Overview

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CWWDL 10817 is a moderately populated, 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, 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 10817 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	–	91.493	25.301	0.267	0.25	-1.653	45.249
Chi et al.	2023	91.507	25.309	0.268	0.279	-1.667	35.468

💡 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	–	–	–	66	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1370	35.1	91.44	25.24	0.27	0.23	-1.6	68.71	0.04

💡 Note: The % column shows the percentage of members that CWWDL 10817 shares with each listed object.

Visualization

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