CWNU 4894

0.27 UTI

0.44

C_N

0.14

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 44

Radius (P>50% members) 2.6 [arcmin]

C_N 0.44 Poorly populated
C_dens 0.14 Very 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 4894 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a very large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~10.53 kpc) differs significantly from the median photometric distance (~15.85 kpc).

Extremely distant Moderate extinction Old

Data

🔍 Search references for CWNU 4894 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	–	282.1	-8.645	0.095	-3.532	-6.758	38.813
He et al.	2023	282.094	-8.641	0.076	-3.561	-6.755	38.81

💡 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	15.85	1.55	–	3981	–	–	–	–

Visualization

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