CWWDL 14442

0.01 UTI

0.62

C_N

0.85

C_dens

1.0

C_C3

0.0

C_lit

0.01

C_dup

C3 classification AA

Number of members (P>50%) 73

Radius (P>50% members) 13.9 [arcmin]

C_N 0.62 Moderately populated
C_dens 0.85 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.01 Very likely duplicate

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

Overview

ℹ️

CWWDL 14442 is a moderately 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 metal-poor, 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.

Metal-poor Young

Data

🔍 Search references for CWWDL 14442 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	283.32	8.177	0.975	-1.319	-3.807	-2.601
Chi et al.	2023	283.328	8.243	0.977	-1.32	-3.804	-9.198

💡 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	–	–	–	50	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 358	98.6	283.31	8.13	0.97	-1.32	-3.81	-3.89	0.1
UPK 50	98.6	283.31	8.14	0.98	-1.32	-3.81	-3.89	0.82

💡 Note: The % column shows the percentage of members that CWWDL 14442 shares with each listed object.

Visualization

ℹ️