CWWDL 13798

0.09 UTI

0.41

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.24

C_dup

C3 classification CB

Number of members (P>50%) 41

Radius (P>50% members) 4.0 [arcmin]

C_N 0.41 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low 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 13798 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, 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 Young

Data

🔍 Search references for CWWDL 13798 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	–	113.858	-18.599	0.41	-1.741	2.407	–
Chi et al.	2023	113.841	-18.583	0.446	-1.807	2.377	122.744

💡 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	–	–	–	38	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2110	100.0	113.86	-18.63	0.4	-1.75	2.41	122.74	0.14
DBSB 7	75.6	113.86	-18.64	0.39	-1.72	2.4	109.31	0.68

💡 Note: The % column shows the percentage of members that CWWDL 13798 shares with each listed object.

Visualization

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