CWNU 3311

0.35 UTI

0.69

C_N

0.33

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 88

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

C_N 0.69 Moderately populated
C_dens 0.33 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 3311 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 moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~11.34 kpc) differs significantly from the median photometric distance (~8.51 kpc).

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3311 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	–	116.076	-40.883	0.088	-1.396	2.858	92.818
He et al.	2023	116.071	-40.884	0.069	-1.4	2.857	95.87

💡 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	8.51	1.05	–	501	–	–	–	–

Visualization

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