CWNU 3036

0.04 UTI

0.29

C_N

0.71

C_dens

0.5

C_C3

0.0

C_lit

0.14

C_dup

C3 classification BB

Number of members (P>50%) 29

Radius (P>50% members) 1.9 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.71 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.14 Likely duplicate

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

Overview

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CWNU 3036 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Low extinction Old

Data

🔍 Search references for CWNU 3036 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	–	110.88	-28.607	0.193	-1.546	2.159	51.868
He et al.	2023	110.888	-28.605	0.194	-1.558	2.155	51.87

💡 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	4.07	0.80	–	1585	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1937	86.2	110.89	-28.61	0.19	-1.54	2.16	51.87	0.38

💡 Note: The % column shows the percentage of members that CWNU 3036 shares with each listed object.

Visualization

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