CWWDL 13493

0.01 UTI

0.41

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.02

C_dup

C3 classification AB

Number of members (P>50%) 41

Radius (P>50% members) 5.2 [arcmin]

C_N 0.41 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

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

Overview

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CWWDL 13493 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a metal-poor, intermediate-age 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.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 13493 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	–	289.432	8.704	0.601	-2.976	-5.269	45.599
Chi et al.	2023	289.419	8.666	0.581	-3.013	-5.263	40.212

💡 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	–	–	–	302	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
PHOC 35	97.6	289.43	8.7	0.6	-2.95	-5.27	44.9	0.58

💡 Note: The % column shows the percentage of members that CWWDL 13493 shares with each listed object.

Visualization

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