CWWDL 14192

0.00 UTI

0.62

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 73

Radius (P>50% members) 6.5 [arcmin]

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high 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 14192 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above 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. 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	–	251.697	-41.21	0.902	1.428	-2.995	-6.307
Chi et al.	2023	251.686	-41.212	0.91	1.42	-3.018	3.301

💡 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	–	–	–	11	0.400	–	–	–

💡 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 33	100.0	251.68	-41.2	0.9	1.4	-3.0	-9.52	0.38
UBC 1561	78.1	251.68	-41.21	0.9	1.45	-2.99	-10.85	0.0
VVVX CL048	65.8	251.69	-41.22	0.9	1.46	-3.0	-10.85	0.5

💡 Note: The % column shows the percentage of members that CWWDL 14192 shares with each listed object.

Visualization

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