CWWDL 14679

0.00 UTI

0.67

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%) 84

Radius (P>50% members) 17.5 [arcmin]

C_N 0.67 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 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14679 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very 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. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14679 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	–	167.445	-76.546	5.201	-22.067	-0.249	14.708
Chi et al.	2023	167.418	-76.444	5.202	-21.884	-0.319	15.051

💡 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	–	–	–	3	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Chamaleon I	100.0	167.16	-77.2	5.25	-22.53	0.29	13.92	0.71
FoF 2435	100.0	167.16	-77.2	5.25	-22.53	0.28	13.92	0.0
OCSN 187	66.7	167.49	-76.53	5.2	-21.84	-0.45	12.25	0.0
OC 0578	59.5	167.51	-76.51	5.19	-21.83	-0.52	12.25	0.0
OCSN 188	19.0	167.09	-77.49	5.29	-23.05	0.59	14.59	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14679 shares with each listed object.

Visualization

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