CWWDL 10880

0.06 UTI

0.67

C_N

0.58

C_dens

0.75

C_C3

0.0

C_lit

0.16

C_dup

C3 classification AB

Number of members (P>50%) 84

Radius (P>50% members) 4.5 [arcmin]

C_N 0.67 Moderately populated
C_dens 0.58 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWWDL 10880 is a moderately populated, moderately dense object of high 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.

⚠️ Warning: This is 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 Young

Data

🔍 Search references for CWWDL 10880 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	–	101.9	5.636	0.243	-0.634	-0.284	93.373
Chi et al.	2023	101.932	5.633	0.268	-0.584	-0.291	111.981

💡 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	–	–	–	44	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1390	84.5	101.89	5.63	0.24	-0.63	-0.29	71.31	0.45
HSC 1638	79.8	101.89	5.63	0.24	-0.64	-0.28	71.31	0.02

💡 Note: The % column shows the percentage of members that CWWDL 10880 shares with each listed object.

Visualization

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