CWWDL 12524

0.02 UTI

0.42

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.05

C_dup

C3 classification AB

Number of members (P>50%) 42

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

C_N 0.42 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

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

Overview

ℹ️

CWWDL 12524 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, 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.

Metal-poor Young

Data

🔍 Search references for CWWDL 12524 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	94.901	26.239	0.287	-0.442	-2.079	8.932
Chi et al.	2023	94.898	26.239	0.281	-0.413	-2.022	17.629

💡 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	–	–	–	87	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 436	95.2	94.9	26.24	0.29	-0.44	-2.08	8.19	0.66

💡 Note: The % column shows the percentage of members that CWWDL 12524 shares with each listed object.

Visualization

ℹ️