CWWDL 13625

0.08 UTI

0.0

C_N

0.34

C_dens

1.0

C_C3

0.0

C_lit

0.28

C_dup

C3 classification AA

Number of members (P>50%) 20

Radius (P>50% members) 5.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.34 Loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

ℹ️

CWWDL 13625 is a sparse, loose object of very high C3 quality. Its parallax locates it at a moderate distance, near 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 possibly a duplicate object, which shares a significant 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 13625 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	251.239	-46.554	0.466	-0.433	-1.632	–
Chi et al.	2023	251.231	-46.562	0.464	-0.398	-1.702	-46.626

💡 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	–	–	–	1	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1555	72.0	251.25	-46.52	0.45	-0.46	-1.58	-47.31	0.59

💡 Note: The % column shows the percentage of members that CWWDL 13625 shares with each listed object.

Visualization

ℹ️