CWWDL 11953

0.02 UTI

0.0

C_N

0.02

C_dens

0.12

C_C3

0.0

C_lit

0.8

C_dup

C3 classification DC

Number of members (P>50%) 13

Radius (P>50% members) 11.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.8 Very likely unique

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

Overview

ℹ️

CWWDL 11953 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, young cluster (see Parameters). It was recently reported in the literature.

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

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.8) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Metal-poor Young

Data

🔍 Search references for CWWDL 11953 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	73.154	48.594	0.292	0.369	-0.939	-3.482
Chi et al.	2023	73.164	48.513	0.317	0.38	-0.917	-4.037

💡 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	–	–	–	81	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2036	20.0	73.15	48.36	0.29	0.54	-1.07	-32.71	0.09

💡 Note: The % column shows the percentage of members that CWWDL 11953 shares with each listed object.

Visualization

ℹ️