CWNU 4075

0.15 UTI

0.0

C_N

0.71

C_dens

0.75

C_C3

0.0

C_lit

0.52

C_dup

C3 classification AB

Number of members (P>50%) 21

Radius (P>50% members) 0.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.71 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

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

Overview

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CWNU 4075 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a very large distance, above the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Very high extinction Very young

Data

🔍 Search references for CWNU 4075 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	–	315.92	49.867	0.096	-2.539	-3.022	–
He et al.	2023	315.922	49.867	0.091	-2.544	-3.022	–

💡 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	9.33	6.15	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 713	48.0	315.94	49.86	0.11	-2.6	-3.08	–	0.11

💡 Note: The % column shows the percentage of members that CWNU 4075 shares with each listed object.

Visualization

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