CWWDL 13502

0.11 UTI

0.46

C_N

0.87

C_dens

1.0

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AA

Number of members (P>50%) 46

Radius (P>50% members) 8.9 [arcmin]

C_N 0.46 Poorly populated
C_dens 0.87 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWWDL 13502 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a metal-poor, very 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.

Metal-poor Very young

Data

🔍 Search references for CWWDL 13502 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	–	318.542	46.375	0.796	-2.97	-3.506	12.289
Chi et al.	2023	318.571	46.39	0.787	-2.981	-3.533	-1.519

💡 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	–	–	–	3	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2561	100.0	318.46	46.38	0.8	-2.96	-3.51	12.29	0.15
UBC 1129	76.1	318.51	46.38	0.79	-2.97	-3.5	2.66	0.38
CWNU 1249	47.8	318.44	46.39	0.8	-2.96	-3.54	19.93	0.06

💡 Note: The % column shows the percentage of members that CWWDL 13502 shares with each listed object.

Visualization

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