CWWDL 14360

0.33 UTI

0.64

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.62

C_dup

C3 classification AA

Number of members (P>50%) 77

Radius (P>50% members) 9.5 [arcmin]

C_N 0.64 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.62 Likely unique

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

Overview

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CWWDL 14360 is a moderately populated, very dense object of very 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.

Note: This is likely a unique object, which shares a moderate 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 14360 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	–	278.511	-13.173	0.921	0.997	0.478	-2.228
Chi et al.	2023	278.493	-13.192	0.928	0.964	0.419	1.696

💡 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	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 984	93.5	278.53	-13.16	0.92	1.0	0.48	2.77	0.08
FoF 2293	37.7	278.45	-13.16	0.92	0.98	0.49	-2.43	0.46

💡 Note: The % column shows the percentage of members that CWWDL 14360 shares with each listed object.

Visualization

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