CWNU 3088

0.08 UTI

0.55

C_N

0.56

C_dens

0.38

C_C3

0.0

C_lit

0.25

C_dup

C3 classification CB

Number of members (P>50%) 59

Radius (P>50% members) 4.5 [arcmin]

C_N 0.55 Moderately populated
C_dens 0.56 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.25 Possibly duplicate

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

Overview

ℹ️

CWNU 3088 is a moderately populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low 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.

Distant Low extinction Very young

Data

🔍 Search references for CWNU 3088 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	121.119	-33.993	0.286	-3.308	4.864	–
He et al.	2023	121.122	-33.988	0.281	-3.307	4.867	–

💡 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	4.79	0.90	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2019	74.6	121.11	-33.99	0.29	-3.29	4.87	–	0.28

💡 Note: The % column shows the percentage of members that CWNU 3088 shares with each listed object.

Visualization

ℹ️