CWWDL 913

0.00 UTI

0.56

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 63

Radius (P>50% members) 2.8 [arcmin]

C_N 0.56 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high 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 913 is a moderately populated, very dense object of very high 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 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 913 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	222.553	-61.76	0.297	-3.441	-1.909	-34.034
Chi et al.	2023	222.547	-61.772	0.295	-3.439	-1.913	-30.22

💡 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	–	–	–	66	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 1314	100.0	222.56	-61.77	0.3	-3.45	-1.92	-33.64	0.55
UBC 1532	100.0	222.56	-61.76	0.3	-3.45	-1.92	-33.64	0.06
OC 0614	39.7	222.55	-61.76	0.3	-3.43	-1.9	-34.03	0.0

💡 Note: The % column shows the percentage of members that CWWDL 913 shares with each listed object.

Visualization

ℹ️