CWNU 3623

0.09 UTI

0.41

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.22

C_dup

C3 classification AC

Number of members (P>50%) 41

Radius (P>50% members) 0.8 [arcmin]

C_N 0.41 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.22 Likely duplicate

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

Overview

ℹ️

CWNU 3623 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large^* distance, above 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~6.09 kpc) differs significantly from the median photometric distance (~8.91 kpc).

Very distant High extinction Very young

Data

🔍 Search references for CWNU 3623 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	17.023	65.646	0.164	-1.84	-0.166	-72.304
He et al.	2023	17.022	65.645	0.168	-1.82	-0.151	-74.3

💡 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	8.91	4.90	–	4	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Pfleiderer 1	78.0	17.02	65.65	0.17	-1.85	-0.13	-74.3	0.43

💡 Note: The % column shows the percentage of members that CWNU 3623 shares with each listed object.

Visualization

ℹ️