CWNU 3130

0.10 UTI

0.5

C_N

0.27

C_dens

0.38

C_C3

0.0

C_lit

0.43

C_dup

C3 classification CB

Number of members (P>50%) 51

Radius (P>50% members) 4.0 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.27 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.43 Possibly duplicate

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

Overview

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CWNU 3130 is a moderately populated, loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age 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.

(*): The parallax distance estimate (~5.28 kpc) differs significantly from the median photometric distance (~3.80 kpc).

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3130 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	99.06	17.16	0.19	0.096	-0.628	32.142
He et al.	2023	99.08	17.16	0.178	0.117	-0.628	32.14

💡 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	3.80	1.40	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1552	56.9	99.13	17.17	0.21	0.05	-0.55	32.14	0.26

💡 Note: The % column shows the percentage of members that CWNU 3130 shares with each listed object.

Visualization

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