CWNU 298

0.16 UTI

0.59

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.34

C_dup

C3 classification AB

Number of members (P>50%) 68

Radius (P>50% members) 3.8 [arcmin]

C_N 0.59 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.34 Possibly duplicate

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

Overview

ℹ️

CWNU 298 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied 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.

(*): The parallax distance estimate (~2.41 kpc) differs significantly from the median photometric distance (~4.37 kpc).

Distant High extinction Metal-rich Very young

Data

🔍 Search references for CWNU 298 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	120.046	-36.723	0.416	-3.126	4.037	24.312
He et al.	2022	120.056	-36.732	0.43	-3.12	4.03	–

💡 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.	2022	4.37	3.60	–	6	0.968	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1431	66.2	120.05	-36.72	0.42	-3.12	4.04	24.31	0.54

💡 Note: The % column shows the percentage of members that CWNU 298 shares with each listed object.

Visualization

ℹ️