CWWDL 10719

0.03 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.0

C_lit

0.92

C_dup

C3 classification DC

Number of members (P>50%) 13

Radius (P>50% members) 7.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.92 Very likely unique

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

Overview

ℹ️

CWWDL 10719 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.92) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 10719 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	78.027	40.773	0.249	0.593	-1.582	-14.041
Chi et al.	2023	78.025	40.766	0.247	0.561	-1.601	-1.095

💡 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	–	–	–	151	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWL 2944	8.0	78.04	40.45	0.26	0.53	-1.51	-13.21	0.05
CWWDL 10773	4.0	78.59	40.59	0.33	0.62	-1.68	-26.79	0.03

💡 Note: The % column shows the percentage of members that CWWDL 10719 shares with each listed object.

Visualization

ℹ️