CWNU 4013

0.32 UTI

0.62

C_N

0.26

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 73

Radius (P>50% members) 2.2 [arcmin]

C_N 0.62 Moderately populated
C_dens 0.26 Loose
C_C3 0.75 High 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 4013 is a moderately populated, loose object of high 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 intermediate-age cluster (see Parameters). It was recently reported in the literature.

Extremely distant Low extinction Intermediate age

Data

🔍 Search references for CWNU 4013 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	–	112.001	-33.864	0.085	-0.725	1.771	–
He et al.	2023	112.004	-33.864	0.075	-0.703	1.771	–

💡 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	10.72	1.00	–	398	–	–	–	–

Visualization

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