CWNU 3385

0.30 UTI

0.51

C_N

0.62

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 52

Radius (P>50% members) 2.8 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.62 Moderately dense
C_C3 0.38 Low 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 3385 is a moderately populated, moderately dense object of low C3 quality. Its parallax locates it at a large^* distance, near 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 (~5.05 kpc) differs significantly from the median photometric distance (~9.12 kpc).

Very distant High extinction Very young

Data

🔍 Search references for CWNU 3385 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	–	28.988	62.103	0.198	-1.481	0.236	–
He et al.	2023	28.966	62.109	0.197	-1.489	0.229	–

💡 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	9.12	3.40	–	10	–	–	–	–

Visualization

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