CWWDL 13357

0.01 UTI

0.42

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%) 42

Radius (P>50% members) 6.2 [arcmin]

C_N 0.42 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 🔍 SciX 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

CWWDL 13357 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 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

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	335.556	54.555	0.663	1.693	-2.306	-9.347
Chi et al.	2023	335.585	54.564	0.658	1.746	-2.368	-8.675

💡 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	–	–	–	54	0.350	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 4535	100.0	335.54	54.55	0.66	1.68	-2.29	-12.31	0.09
HXHWL 23	97.6	335.54	54.56	0.66	1.68	-2.29	-12.31	0.46

💡 Note: The % column shows the percentage of members that CWWDL 13357 shares with each listed object.

Visualization

💡 Note: How are the galactocentric plots generated? See FAQ.