CWNU 3760

0.16 UTI

0.32

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.44

C_dup

C3 classification BB

Number of members (P>50%) 32

Radius (P>50% members) 1.8 [arcmin]

C_N 0.32 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

ℹ️

CWNU 3760 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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.

Distant Moderate extinction Very young

Data

🔍 Search references for CWNU 3760 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	114.8	-18.942	0.261	-1.758	2.33	67.756
He et al.	2023	114.796	-18.944	0.246	-1.764	2.328	–

💡 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	3.63	1.40	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1866	56.2	114.8	-18.94	0.27	-1.73	2.31	67.76	0.2

💡 Note: The % column shows the percentage of members that CWNU 3760 shares with each listed object.

Visualization

ℹ️