CWWDL 3247

0.28 UTI

0.28

C_N

1.0

C_dens

0.12

C_C3

0.0

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 28

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

C_N 0.28 Poorly populated
C_dens 1.0 Very dense
C_C3 0.12 Very low 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 3247 is a poorly populated, very dense object of very low C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 3247 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	–	229.357	-21.008	0.23	-5.351	-3.505	–
Chi et al.	2023	229.359	-21.001	0.3	-5.365	-3.534	–

💡 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	–	–	–	76	0.070	–	–	–

Visualization

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