CWNU 4088

0.06 UTI

0.32

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.16

C_dup

C3 classification BA

Number of members (P>50%) 32

Radius (P>50% members) 2.8 [arcmin]

C_N 0.32 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWNU 4088 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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.

⚠️ 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 Very high extinction Very young

Data

🔍 Search references for CWNU 4088 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	–	268.44	-25.109	0.322	-0.166	-2.093	102.643
He et al.	2023	268.436	-25.11	0.319	-0.166	-2.09	–

💡 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	3.63	5.30	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 56	84.4	268.44	-25.11	0.33	-0.23	-2.12	-5.15	0.39

💡 Note: The % column shows the percentage of members that CWNU 4088 shares with each listed object.

Visualization

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