CWNU 3349

0.38 UTI

0.46

C_N

0.8

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 46

Radius (P>50% members) 1.0 [arcmin]

C_N 0.46 Poorly populated
C_dens 0.8 Dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 3349 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well above the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~11.68 kpc) differs significantly from the median photometric distance (~20.89 kpc).

Extremely distant High extinction Very young

Data

🔍 Search references for CWNU 3349 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	–	323.804	57.102	0.086	-1.951	-2.05	-83.534
He et al.	2023	323.806	57.098	0.068	-1.937	-2.037	–

💡 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	20.89	3.95	–	2	–	–	–	–

Visualization

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