CWNU 4193

0.36 UTI

0.52

C_N

0.53

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 53

Radius (P>50% members) 1.0 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.53 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

ℹ️

CWNU 4193 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~15.36 kpc) differs significantly from the median photometric distance (~23.99 kpc).

Extremely distant High extinction Intermediate age

Data

🔍 Search references for CWNU 4193 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	121.169	-38.919	0.065	-0.751	1.619	140.153
He et al.	2023	121.181	-38.917	0.065	-0.763	1.596	–

💡 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	23.99	3.30	–	794	–	–	–	–

Visualization

ℹ️