CWNU 3619

0.23 UTI

0.27

C_N

0.52

C_dens

0.75

C_C3

0.0

C_lit

0.74

C_dup

C3 classification BA

Number of members (P>50%) 27

Radius (P>50% members) 3.4 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.52 Moderately 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 3619 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a 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 Moderate extinction Young

Data

🔍 Search references for CWNU 3619 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	–	316.808	47.258	0.308	-3.421	-4.413	–
He et al.	2023	316.805	47.255	0.287	-3.421	-4.424	–

💡 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	3.02	1.30	–	20	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1775	25.9	316.74	47.15	0.3	-3.38	-4.35	–	0.03

💡 Note: The % column shows the percentage of members that CWNU 3619 shares with each listed object.

Visualization

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