CWWDL 13945

0.00 UTI

0.4

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CB

Number of members (P>50%) 40

Radius (P>50% members) 5.1 [arcmin]

C_N 0.4 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

CWWDL 13945 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very 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, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	330.471	56.029	0.641	-2.004	-1.667	34.448
Chi et al.	2023	330.475	56.025	0.627	-2.014	-1.697	-14.965

💡 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	–	–	–	10	-0.280	–	–	–

💡 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
HXHWL 28	100.0	330.47	56.03	0.64	-2.01	-1.66	34.45	0.51
UBC 1154	100.0	330.47	56.04	0.64	-2.0	-1.67	34.45	0.01
CWWDL 14210	92.5	330.47	56.05	0.64	-1.98	-1.7	34.45	0.13

💡 Note: The % column shows the percentage of members that CWWDL 13945 shares with each listed object.

Visualization

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