CWNU 3589

0.27 UTI

0.58

C_N

0.13

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 67

Radius (P>50% members) 3.9 [arcmin]

C_N 0.58 Moderately populated
C_dens 0.13 Very loose
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 3589 is a moderately populated, very loose 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 (~8.84 kpc) differs significantly from the median photometric distance (~6.46 kpc).

Very distant High extinction Intermediate age

Data

🔍 Search references for CWNU 3589 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	–	355.959	62.858	0.113	-1.584	-0.276	-53.153
He et al.	2023	355.962	62.861	0.112	-1.587	-0.267	-28.68

💡 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	6.46	3.15	–	794	–	–	–	–

Visualization

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