CWNU 4799

0.04 UTI

0.0

C_N

0.71

C_dens

0.62

C_C3

0.0

C_lit

0.16

C_dup

C3 classification CA

Number of members (P>50%) 20

Radius (P>50% members) 1.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.71 Moderately dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 4799 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Low extinction Very young

Data

🔍 Search references for CWNU 4799 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	–	298.672	29.799	0.233	-2.454	-4.849	–
He et al.	2023	298.663	29.801	0.228	-2.446	-4.852	–

💡 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	3.98	0.05	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 529	84.0	298.67	29.79	0.23	-2.46	-4.84	–	0.2
FoF 1728	36.0	298.73	29.91	0.23	-2.41	-4.87	–	0.11

💡 Note: The % column shows the percentage of members that CWNU 4799 shares with each listed object.

Visualization

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