CWWDL 13990

0.01 UTI

0.35

C_N

0.82

C_dens

1.0

C_C3

0.0

C_lit

0.03

C_dup

N₅₀ (P>50% members) 35

Stellar density (N₅₀/rad) 4.1 [N/pc²]

C3 classification AA

C_N 0.35 Poorly populated
C_dens 0.82 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 13990 is a poorly populated, 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

🔍 Search references for CWWDL 13990 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	99999–	273.109	-15.381	0.587	-0.247	-1.773	27.729
Chi et al.	2023	273.123	-15.368	0.589	-0.213	-1.814	10.258

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	1	-0.180	–	–	–
Chi et al.	2023	–	–	–	1	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1013	97.1	273.11	-15.38	0.58	-0.23	-1.74	32.92	0.1
HXHWL 66	77.1	273.12	-15.38	0.58	-0.24	-1.74	2.21	0.51

💡 Note: The % column shows the percentage of members that CWWDL 13990 shares with each listed object.

Visualization

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