CWWDL 13298

0.00 UTI

0.47

C_N

0.57

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 47

Radius (P>50% members) 6.6 [arcmin]

C_N 0.47 Poorly populated
C_dens 0.57 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 13298 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, very young 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 Very young

Data

🔍 Search references for CWWDL 13298 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	–	102.73	-9.982	0.473	-1.305	1.242	–
Chi et al.	2023	102.736	-9.954	0.482	-1.326	1.24	–

💡 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	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 61	100.0	102.73	-9.97	0.48	-1.29	1.24	–	0.5
Theia 2266	100.0	102.73	-9.99	0.48	-1.3	1.24	–	0.01
UBC 1354	100.0	102.73	-9.98	0.48	-1.3	1.24	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 13298 shares with each listed object.

Visualization

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