CWNU 3600

0.37 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.74

C_dup

C3 classification AB

Number of members (P>50%) 105

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

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.74 Likely unique

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

Overview

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CWNU 3600 is a rich, 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.

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.

Distant Very high extinction Very young

Data

🔍 Search references for CWNU 3600 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	–	269.595	-24.555	0.333	-0.229	-0.687	-15.504
He et al.	2023	269.591	-24.556	0.328	-0.231	-0.69	-15.47

💡 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	3.89	5.90	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 72	25.7	269.59	-24.56	0.31	-0.24	-0.69	-649.85	0.45

💡 Note: The % column shows the percentage of members that CWNU 3600 shares with each listed object.

Visualization

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