CWNU 3815

0.13 UTI

0.52

C_N

0.66

C_dens

0.5

C_C3

0.0

C_lit

0.38

C_dup

C3 classification BB

Number of members (P>50%) 53

Radius (P>50% members) 2.4 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.66 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.38 Possibly duplicate

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

Overview

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CWNU 3815 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported 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.

Very distant High extinction Young

Data

🔍 Search references for CWNU 3815 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	–	141.099	-53.22	0.175	-4.312	3.925	80.656
He et al.	2023	141.098	-53.22	0.175	-4.287	3.927	60.52

💡 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	6.31	3.25	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch J0924.3-5313	62.3	141.1	-53.22	0.17	-4.31	3.93	60.52	0.42

💡 Note: The % column shows the percentage of members that CWNU 3815 shares with each listed object.

Visualization

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