CWNU 363

0.23 UTI

0.66

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.47

C_dup

C3 classification AB

Number of members (P>50%) 83

Radius (P>50% members) 6.1 [arcmin]

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.47 Possibly duplicate

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

Overview

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CWNU 363 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Very young

Data

🔍 Search references for CWNU 363 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	–	121.214	-39.159	1.125	-4.583	3.985	25.423
He et al.	2022	121.197	-39.182	1.128	-4.586	3.989	–
He et al.	2022	121.209	-39.174	1.13	-4.58	3.97	–

💡 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.	2022	–	1.05	–	6	–	–	–	–
He et al.	2022	0.81	0.84	–	8	0.169	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0446	53.0	121.2	-39.2	1.13	-4.57	3.96	24.14	0.59

💡 Note: The % column shows the percentage of members that CWNU 363 shares with each listed object.

Visualization

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