CWNU 3597

0.43 UTI

0.58

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.84

C_dup

C3 classification AA

Number of members (P>50%) 67

Radius (P>50% members) 3.5 [arcmin]

C_N 0.58 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.84 Very likely unique

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

Overview

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CWNU 3597 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Very young

Data

🔍 Search references for CWNU 3597 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	–	207.691	-62.865	0.299	-6.674	-1.879	-61.792
He et al.	2023	207.713	-62.87	0.299	-6.673	-1.877	29.49

💡 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	5.00	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2612	16.4	207.43	-62.88	0.3	-6.39	-1.98	7.21	0.37

💡 Note: The % column shows the percentage of members that CWNU 3597 shares with each listed object.

Visualization

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