CWNU 4134

0.29 UTI

0.66

C_N

0.46

C_dens

0.5

C_C3

0.0

C_lit

0.9

C_dup

C3 classification BB

Number of members (P>50%) 82

Radius (P>50% members) 6.7 [arcmin]

C_N 0.66 Moderately populated
C_dens 0.46 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.9 Very likely unique

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

Overview

ℹ️

CWNU 4134 is a moderately populated, 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 very young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Very young

Data

🔍 Search references for CWNU 4134 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	275.418	-15.846	0.327	-0.58	-1.972	31.837
He et al.	2023	275.457	-15.855	0.343	-0.595	-1.967	6.54

💡 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	3.09	4.45	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 186	9.8	275.43	-15.8	0.32	-0.47	-2.28	28.35	0.21

💡 Note: The % column shows the percentage of members that CWNU 4134 shares with each listed object.

Visualization

ℹ️