CWWDL 13348

0.00 UTI

0.33

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CA

Number of members (P>50%) 33

Radius (P>50% members) 3.7 [arcmin]

C_N 0.33 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

ℹ️

CWWDL 13348 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near 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 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.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13348 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	259.264	-41.704	0.6	-0.025	-3.591	-39.283
Chi et al.	2023	259.283	-41.682	0.591	0.015	-3.574	-60.5

💡 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	–	–	–	62	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1563	100.0	259.26	-41.7	0.6	-0.05	-3.59	-30.23	0.65
CWNU 1	81.8	259.27	-41.69	0.6	-0.04	-3.59	-30.23	0.0

💡 Note: The % column shows the percentage of members that CWWDL 13348 shares with each listed object.

Visualization

ℹ️