CWWDL 13365

0.05 UTI

0.3

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.13

C_dup

C3 classification BB

Number of members (P>50%) 30

Radius (P>50% members) 3.6 [arcmin]

C_N 0.3 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.13 Likely duplicate

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

Overview

ℹ️

CWWDL 13365 is a poorly populated, very dense 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, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is 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 13365 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	16.486	59.627	0.497	-1.163	-0.477	-51.505
Chi et al.	2023	16.433	59.657	0.499	-1.233	-0.511	-51.505

💡 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	–	–	–	44	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 36	86.7	16.49	59.63	0.5	-1.16	-0.45	-51.5	0.6

💡 Note: The % column shows the percentage of members that CWWDL 13365 shares with each listed object.

Visualization

ℹ️