CWNU 3529

0.51 UTI

0.68

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.94

C_dup

C3 classification AA

Number of members (P>50%) 87

Radius (P>50% members) 3.8 [arcmin]

C_N 0.68 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.94 Very likely unique

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

Overview

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CWNU 3529 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 very small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 3529 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	–	263.428	-35.016	0.355	-0.814	-2.324	-33.331
He et al.	2023	263.436	-35.01	0.359	-0.804	-2.323	9.94

💡 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	2.29	3.60	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2921	5.7	263.44	-35.01	0.38	-0.63	-2.08	118.22	0.09
UFMG 87	1.1	263.3	-35.13	0.29	-1.02	-2.73	-17.61	0.65

💡 Note: The % column shows the percentage of members that CWNU 3529 shares with each listed object.

Visualization

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