CWNU 3498

0.12 UTI

0.26

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.35

C_dup

C3 classification BB

Number of members (P>50%) 26

Radius (P>50% members) 1.1 [arcmin]

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.35 Possibly duplicate

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

Overview

ℹ️

CWNU 3498 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate 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.

⚠️ 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.

Relatively close Very high extinction Young

Data

🔍 Search references for CWNU 3498 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	287.611	10.309	0.331	-1.178	-3.492	123.319
He et al.	2023	287.61	10.309	0.333	-1.152	-3.479	123.32

💡 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	2.40	5.60	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 148	65.4	287.61	10.31	0.31	-1.22	-3.5	50.93	0.3

💡 Note: The % column shows the percentage of members that CWNU 3498 shares with each listed object.

Visualization

ℹ️