CWNU 3641

0.11 UTI

0.4

C_N

0.45

C_dens

0.5

C_C3

0.0

C_lit

0.4

C_dup

C3 classification BB

Number of members (P>50%) 40

Radius (P>50% members) 5.6 [arcmin]

C_N 0.4 Poorly populated
C_dens 0.45 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.4 Possibly duplicate

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

Overview

ℹ️

CWNU 3641 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate 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.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Very young

Data

🔍 Search references for CWNU 3641 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	160.522	-58.438	0.388	-7.166	2.948	-97.606
He et al.	2023	160.498	-58.443	0.38	-7.169	2.948	–

💡 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
He et al.	2023	2.82	1.70	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2358	60.0	160.5	-58.44	0.38	-7.16	2.95	–	0.22

💡 Note: The % column shows the percentage of members that CWNU 3641 shares with each listed object.

Visualization

ℹ️