CWWDL 13799

0.01 UTI

0.26

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.04

C_dup

C3 classification BB

Number of members (P>50%) 26

Radius (P>50% members) 3.0 [arcmin]

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

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

Overview

ℹ️

CWWDL 13799 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, very 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 Very young

Data

🔍 Search references for CWWDL 13799 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	114.95	-18.923	0.436	-2.231	2.217	–
Chi et al.	2023	114.981	-18.983	0.449	-2.199	2.178	–

💡 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	–	–	–	4	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 59	96.2	114.95	-18.92	0.42	-2.24	2.22	–	0.42
UBC 1381	92.3	114.95	-18.92	0.43	-2.24	2.22	–	0.01

💡 Note: The % column shows the percentage of members that CWWDL 13799 shares with each listed object.

Visualization

ℹ️