CWWL 3595

0.00 UTI

0.66

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 81

Stellar density (N₅₀/rad) 21.0 [N/pc²]

C3 classification AA

C_N 0.66 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

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWL 3595 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane. It is catalogued as a metal-rich, 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.

Metal-rich Intermediate age

Data

🔍 Search references for CWWL 3595 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	99999–	282.533	33.371	3.469	1.822	-3.874	-18.538
Chi et al.	2023	282.582	33.407	3.497	1.815	-3.878	–

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	275	0.537	–	–	–
Chi et al.	2023	–	–	–	275	0.537	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Gaia 8	100.0	282.56	33.36	3.45	1.79	-3.89	-18.69	0.67
OCSN 249	100.0	282.52	33.39	3.46	1.82	-3.87	-18.83	0.0
PHOC 41	100.0	282.54	33.38	3.45	1.8	-3.86	-18.69	0.0

💡 Note: The % column shows the percentage of members that CWWL 3595 shares with each listed object.

Visualization

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