CWNU 3030

0.19 UTI

0.6

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.39

C_dup

C3 classification AB

Number of members (P>50%) 71

Radius (P>50% members) 1.3 [arcmin]

C_N 0.6 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.39 Possibly duplicate

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

Overview

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CWNU 3030 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large^* distance, below 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 (~8.84 kpc) differs significantly from the median photometric distance (~6.46 kpc).

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3030 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	–	315.741	44.497	0.113	-2.897	-3.039	-72.05
He et al.	2023	315.742	44.499	0.096	-2.884	-3.047	-72.05

💡 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	6.46	2.80	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Collinder 428	60.6	315.74	44.5	0.1	-2.91	-3.04	-86.07	0.59

💡 Note: The % column shows the percentage of members that CWNU 3030 shares with each listed object.

Visualization

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