CWWDL 13311

0.09 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.17

C_dup

C3 classification AB

Number of members (P>50%) 106

Radius (P>50% members) 7.4 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

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

Overview

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CWWDL 13311 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 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 13311 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	–	153.17	-60.899	0.491	-6.356	3.114	-11.967
Chi et al.	2023	153.153	-60.923	0.498	-6.335	3.165	-10.043

💡 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	–	–	–	31	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2059	83.0	153.21	-60.91	0.49	-6.36	3.08	-11.96	0.65
UBC 257	77.4	153.19	-60.9	0.49	-6.35	3.08	-11.9	0.03
OC 0540	53.8	153.19	-60.93	0.5	-6.34	3.09	-11.9	0.01

💡 Note: The % column shows the percentage of members that CWWDL 13311 shares with each listed object.

Visualization

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