CWNU 3537

0.03 UTI

0.52

C_N

0.19

C_dens

0.75

C_C3

0.0

C_lit

0.11

C_dup

C3 classification AB

Number of members (P>50%) 53

Radius (P>50% members) 4.9 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.19 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.11 Likely duplicate

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

Overview

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CWNU 3537 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a large 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.

⚠️ 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.

Very distant High extinction Very young

Data

🔍 Search references for CWNU 3537 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	–	155.614	-58.116	0.19	-5.55	3.17	66.673
He et al.	2023	155.612	-58.123	0.184	-5.589	3.162	–

💡 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	5.50	3.80	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2332	88.7	155.6	-58.12	0.18	-5.55	3.17	66.67	0.31

💡 Note: The % column shows the percentage of members that CWNU 3537 shares with each listed object.

Visualization

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