CWWDL 1713

0.48 UTI

0.42

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 42

Radius (P>50% members) 1.2 [arcmin]

C_N 0.42 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWWDL 1713 is a poorly populated, very dense object of very high 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 object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Metal-poor Young

Data

🔍 Search references for CWWDL 1713 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	–	274.412	-16.36	0.303	-0.534	-1.03	40.357
Chi et al.	2023	274.415	-16.357	0.313	-0.527	-1.019	40.357

💡 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	–	–	–	33	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3264	100.0	274.41	-16.36	0.3	-0.53	-1.05	41.11	0.18
HSC 178	97.6	274.41	-16.36	0.32	-0.53	-1.03	41.19	0.07

💡 Note: The % column shows the percentage of members that CWWDL 1713 shares with each listed object.

Visualization

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