CWNU 2630

0.11 UTI

0.34

C_N

0.43

C_dens

0.75

C_C3

0.0

C_lit

0.35

C_dup

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 5.5 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.43 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.35 Possibly duplicate

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

Overview

ℹ️

CWNU 2630 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a 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.

Relatively close High extinction Young

Data

🔍 Search references for CWNU 2630 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	291.356	11.638	0.401	-2.067	-4.25	52.897
He et al.	2023	291.344	11.623	0.41	-2.066	-4.26	37.77

💡 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	2.24	4.90	–	71	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Dolidze 35	64.7	291.35	11.63	0.39	-2.07	-4.26	22.65	0.38

💡 Note: The % column shows the percentage of members that CWNU 2630 shares with each listed object.

Visualization

ℹ️