CWWDL 13298

0.00 UTI

0.47

C_N

0.57

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 47

Radius (P>50% members) 6.6 [arcmin]

C_N 0.47 Poorly populated
C_dens 0.57 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

CWWDL 13298 is a poorly populated, moderately dense object of high 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.

⚠️ 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

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	102.73	-9.982	0.473	-1.305	1.242	–
Chi et al.	2023	102.736	-9.954	0.482	-1.326	1.24	–

💡 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	–	–	–	18	0.270	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 61	100.0	102.73	-9.97	0.48	-1.29	1.24	–	0.5
Theia 2266	100.0	102.73	-9.99	0.48	-1.3	1.24	–	0.01
UBC 1354	100.0	102.73	-9.98	0.48	-1.3	1.24	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 13298 shares with each listed object.

Visualization

💡 Note: How are the galactocentric plots generated? See FAQ.