CWNU 2501

0.03 UTI

0.56

C_N

0.71

C_dens

0.5

C_C3

0.0

C_lit

0.1

C_dup

C3 classification BB

Number of members (P>50%) 63

Radius (P>50% members) 6.5 [arcmin]

C_N 0.56 Moderately populated
C_dens 0.71 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.1 Likely duplicate

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

Overview

ℹ️

CWNU 2501 is a moderately populated, 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 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.

Relatively close Low extinction Young

Data

🔍 Search references for CWNU 2501 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	105.362	-3.141	0.448	-1.22	0.597	56.53
He et al.	2023	105.354	-3.162	0.455	-1.186	0.583	–

💡 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	2.00	0.75	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Wit 2	90.5	105.35	-3.13	0.43	-1.23	0.57	56.53	0.67
Ferrero 10	30.2	105.19	-3.05	0.44	-1.29	0.64	83.93	0.31

💡 Note: The % column shows the percentage of members that CWNU 2501 shares with each listed object.

Visualization

ℹ️