CWNU 2599

0.12 UTI

0.38

C_N

0.71

C_dens

0.75

C_C3

0.0

C_lit

0.32

C_dup

C3 classification AB

Number of members (P>50%) 38

Radius (P>50% members) 3.1 [arcmin]

C_N 0.38 Poorly populated
C_dens 0.71 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWNU 2599 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Very young

Data

🔍 Search references for CWNU 2599 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	–	186.73	-62.822	0.275	-6.132	-0.356	-25.346
He et al.	2023	186.748	-62.824	0.286	-6.131	-0.364	–

💡 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	3.09	4.45	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
MCM 32	68.4	186.73	-62.83	0.27	-6.14	-0.35	-25.35	0.37

💡 Note: The % column shows the percentage of members that CWNU 2599 shares with each listed object.

Visualization

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