CWWDL 13542

0.04 UTI

0.0

C_N

0.14

C_dens

0.12

C_C3

0.0

C_lit

0.72

C_dup

C3 classification DC

Number of members (P>50%) 17

Radius (P>50% members) 7.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.14 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.72 Likely unique

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

Overview

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CWWDL 13542 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a metal-poor, 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.

Metal-poor Young

Data

🔍 Search references for CWWDL 13542 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	–	117.146	-25.316	0.439	-1.568	1.379	26.732
Chi et al.	2023	117.163	-25.313	0.447	-1.535	1.449	–

💡 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	–	–	–	93	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 9	28.0	117.11	-25.38	0.4	-1.61	1.27	26.73	0.17
Theia 3628	20.0	117.16	-25.42	0.41	-1.6	1.28	26.73	0.03

💡 Note: The % column shows the percentage of members that CWWDL 13542 shares with each listed object.

Visualization

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