CWWL 3512

0.51 UTI

0.76

C_N

0.81

C_dens

1.0

C_C3

0.0

C_lit

0.99

C_dup

C3 classification AA

Number of members (P>50%) 128

Radius (P>50% members) 56.6 [arcmin]

C_N 0.76 Rich
C_dens 0.81 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.99 Unique

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

Overview

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CWWL 3512 is a rich, dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWL 3512 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	80.71	-1.295	2.923	1.281	-0.362	16.238
Chi et al.	2023	80.643	-1.214	2.923	1.26	-0.443	–

💡 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	–	–	–	170	-0.082	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14536	7.0	79.78	-1.29	2.73	1.52	-0.49	17.25	0.32
ASCC 16	0.8	81.23	1.65	2.87	1.39	-0.09	18.3	1.0

💡 Note: The % column shows the percentage of members that CWWL 3512 shares with each listed object.

Visualization

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