CWNU 3677

0.25 UTI

0.3

C_N

0.2

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 30

Core radius and density 1.6 [pc], 1.0 [pc^-2]

C3 classification BA

C_N 0.3 Poorly populated
C_dens 0.2 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3677 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Very distant Moderate extinction Very young

Data

🔍 Search references for CWNU 3677 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–	115.005	-23.512	0.161	-1.536	2.393	81.784
He et al.	2023	115.007	-23.514	0.142	-1.537	2.39	–

💡 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–	5.25	1.45	–	16	–	–	–	–
He et al.	2023	5.25	1.45	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Pickard 160	66.7	115.01	-23.52	0.15	-1.52	2.36	59.58	0.05

💡 Note: The % column shows the percentage of members that CWNU 3677 shares with each listed object.

Visualization

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