CWNU 2395

0.35 UTI

0.56

C_N

0.43

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 63

Radius (P>50% members) 7.1 [arcmin]

C_N 0.56 Moderately populated
C_dens 0.43 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 2395 is a moderately populated, loose 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.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 2395 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	–	245.655	-49.169	0.38	-1.423	-2.927	-27.985
He et al.	2023	245.649	-49.19	0.405	-1.424	-2.925	-3.71

💡 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	2.40	3.15	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2776	11.1	246.06	-48.86	0.36	-1.36	-2.85	-34.7	0.16

💡 Note: The % column shows the percentage of members that CWNU 2395 shares with each listed object.

Visualization

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