CWNU 3335

0.27 UTI

0.25

C_N

0.6

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 25

Radius (P>50% members) 1.1 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.6 Moderately dense
C_C3 0.5 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 3335 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~9.01 kpc) differs significantly from the median photometric distance (~5.13 kpc).

Very distant High extinction Intermediate age

Data

🔍 Search references for CWNU 3335 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	–	298.337	30.882	0.111	-3.056	-5.47	-48.318
He et al.	2023	298.336	30.886	0.126	-3.048	-5.466	-49.16

💡 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	5.13	3.30	–	794	–	–	–	–

Visualization

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