CWWDL 13433

0.04 UTI

0.37

C_N

0.98

C_dens

1.0

C_C3

0.0

C_lit

0.08

C_dup

C3 classification AA

Number of members (P>50%) 37

Radius (P>50% members) 4.2 [arcmin]

C_N 0.37 Poorly populated
C_dens 0.98 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

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

Overview

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CWWDL 13433 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 near-solar metallicity, young 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.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13433 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	–	216.444	-61.913	0.444	-4.082	-2.724	-47.571
Chi et al.	2023	216.356	-61.91	0.445	-4.038	-2.748	-28.651

💡 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	–	–	–	44	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1525	91.9	216.46	-61.9	0.45	-4.1	-2.72	-47.57	0.6

💡 Note: The % column shows the percentage of members that CWWDL 13433 shares with each listed object.

Visualization

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