CWWL 3526

0.00 UTI

0.5

C_N

0.4

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 50

Radius (P>50% members) 43.7 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.4 Loose
C_C3 1.0 Very 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

CWWL 3526 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age 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 Intermediate age

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	117.913	-46.814	2.539	-4.782	8.825	19.737
Chi et al.	2023	118.28	-47.348	2.521	-4.886	8.762	–

💡 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	–	–	–	148	0.051	–	–	–

💡 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
FoF 2387	100.0	117.39	-46.67	2.53	-4.71	8.96	17.63	0.52
OCSN 200	100.0	117.36	-46.54	2.54	-4.69	9.01	17.63	0.04
OC 0470	38.0	117.34	-46.37	2.55	-4.71	9.06	17.63	0.64
CWWDL 14576	6.0	116.76	-47.37	2.52	-4.68	8.88	20.47	0.0

💡 Note: The % column shows the percentage of members that CWWL 3526 shares with each listed object.

Visualization

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