CWWDL 14487

0.01 UTI

0.0

C_N

0.18

C_dens

0.5

C_C3

0.0

C_lit

0.08

C_dup

C3 classification BB

Number of members (P>50%) 22

Radius (P>50% members) 16.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.18 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

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

Overview

ℹ️

CWWDL 14487 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a near-solar metallicity, 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 Young

Data

🔍 Search references for CWWDL 14487 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	9.185	68.831	0.989	-1.515	-0.625	-16.4
Chi et al.	2023	9.291	68.84	0.981	-1.555	-0.724	-9.997

💡 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	–	–	–	23	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 39	92.0	9.19	68.83	0.98	-1.51	-0.63	-16.4	0.13
Theia 2175	80.0	8.72	68.84	0.98	-1.53	-0.65	-18.21	0.04

💡 Note: The % column shows the percentage of members that CWWDL 14487 shares with each listed object.

Visualization

ℹ️