CWWDL 10236

0.02 UTI

0.48

C_N

0.86

C_dens

0.5

C_C3

0.0

C_lit

0.04

C_dup

C3 classification BB

Number of members (P>50%) 48

Radius (P>50% members) 4.4 [arcmin]

C_N 0.48 Poorly populated
C_dens 0.86 Dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

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

Overview

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CWWDL 10236 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 10236 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	–	303.618	37.406	0.384	-1.326	-3.158	-3.403
Chi et al.	2023	303.608	37.425	0.397	-1.331	-3.161	-3.403

💡 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	–	–	–	115	-0.040	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 248	95.8	303.62	37.4	0.38	-1.3	-3.14	-3.4	0.04
UBC 1097	93.8	303.63	37.41	0.37	-1.31	-3.15	-3.4	0.5

💡 Note: The % column shows the percentage of members that CWWDL 10236 shares with each listed object.

Visualization

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