CWNU 3029

0.20 UTI

0.0

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.56

C_dup

C3 classification AB

Number of members (P>50%) 22

Radius (P>50% members) 0.7 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.56 Likely unique

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

Overview

ℹ️

CWNU 3029 is a sparse, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

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

Very distant Very high extinction Young

Data

🔍 Search references for CWNU 3029 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	178.319	-62.609	0.119	-6.44	1.167	-0.094
He et al.	2023	178.315	-62.607	0.136	-6.418	1.171	-16.6

💡 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	7.59	5.15	–	63	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
MCM 26	44.0	178.31	-62.6	0.13	-6.52	1.13	-18.83	0.23

💡 Note: The % column shows the percentage of members that CWNU 3029 shares with each listed object.

Visualization

ℹ️