CWNU 3914

0.04 UTI

0.0

C_N

0.04

C_dens

0.62

C_C3

0.0

C_lit

0.28

C_dup

C3 classification AC

Number of members (P>50%) 20

Radius (P>50% members) 1.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

ℹ️

CWNU 3914 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a very large distance, above the mid-plane, affected by very high 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.

Extremely distant Very high extinction Very young

Data

🔍 Search references for CWNU 3914 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	291.252	17.546	0.048	-2.844	-5.866	23.039
He et al.	2023	291.259	17.55	0.059	-2.832	-5.906	19.75

💡 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	29.51	8.65	–	3	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 431	72.0	291.26	17.54	0.07	-2.81	-5.88	23.04	0.17

💡 Note: The % column shows the percentage of members that CWNU 3914 shares with each listed object.

Visualization

ℹ️