CWWDL 14116

0.28 UTI

0.65

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.52

C_dup

C3 classification AA

Number of members (P>50%) 80

Radius (P>50% members) 8.3 [arcmin]

C_N 0.65 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

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

Overview

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CWWDL 14116 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14116 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	–	281.317	-11.089	0.743	-1.112	-3.389	6.726
Chi et al.	2023	281.346	-11.142	0.76	-1.123	-3.382	32.715

💡 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	–	–	–	15	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14115	53.8	281.27	-11.05	0.74	-1.08	-3.38	28.47	0.12
UBC 100	47.5	281.24	-11.09	0.73	-1.1	-3.37	40.12	0.66

💡 Note: The % column shows the percentage of members that CWWDL 14116 shares with each listed object.

Visualization

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