CWWDL 13361

0.20 UTI

0.27

C_N

0.17

C_dens

0.62

C_C3

0.0

C_lit

0.96

C_dup

C3 classification AC

Number of members (P>50%) 27

Radius (P>50% members) 8.8 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.17 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

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

Overview

ℹ️

CWWDL 13361 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry, and a 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=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 13361 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	34.892	58.77	0.449	-0.756	-0.703	-18.967
Chi et al.	2023	34.878	58.77	0.461	-0.698	-0.694	-30.602

💡 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	–	–	–	1	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 13519	14.8	35.07	59.03	0.42	-0.76	-0.69	–	0.14
UBC 419	3.7	34.61	58.98	0.4	-0.92	-0.66	–	0.32

💡 Note: The % column shows the percentage of members that CWWDL 13361 shares with each listed object.

Visualization

ℹ️