CWNU 3787

0.00 UTI

0.0

C_N

0.23

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BB

Number of members (P>50%) 23

Radius (P>50% members) 3.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.23 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

ℹ️

CWNU 3787 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a young 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.

Distant High extinction Young

Data

🔍 Search references for CWNU 3787 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	185.53	-62.306	0.235	-6.488	0.413	72.515
He et al.	2023	185.485	-62.294	0.237	-6.486	0.43	–

💡 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	3.89	5.00	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2506	100.0	185.53	-62.31	0.24	-6.49	0.42	31.11	0.25
FoF 1595	8.0	185.66	-62.43	0.25	-6.62	0.38	-25.58	0.03

💡 Note: The % column shows the percentage of members that CWNU 3787 shares with each listed object.

Visualization

ℹ️