CWNU 3313

0.28 UTI

0.5

C_N

0.77

C_dens

0.38

C_C3

0.0

C_lit

0.86

C_dup

C3 classification BC

Number of members (P>50%) 50

Radius (P>50% members) 0.8 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.77 Dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.86 Very likely unique

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

Overview

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CWNU 3313 is a moderately populated, dense object of low C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~15.53 kpc) differs significantly from the median photometric distance (~10.47 kpc).

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Extremely distant Low extinction Old

Data

🔍 Search references for CWNU 3313 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	–	151.39	-61.043	0.064	-3.633	2.342	–
He et al.	2023	151.387	-61.042	0.059	-3.633	2.319	–

💡 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	10.47	0.80	–	1585	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 69	14.0	151.5	-61.05	0.11	-3.66	2.39	–	0.05

💡 Note: The % column shows the percentage of members that CWNU 3313 shares with each listed object.

Visualization

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