CWNU 4436

0.04 UTI

0.33

C_N

0.38

C_dens

0.12

C_C3

0.0

C_lit

0.21

C_dup

C3 classification DC

Number of members (P>50%) 33

Radius (P>50% members) 3.3 [arcmin]

C_N 0.33 Poorly populated
C_dens 0.38 Loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

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

Overview

ℹ️

CWNU 4436 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age 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.

Very distant High extinction Intermediate age

Data

🔍 Search references for CWNU 4436 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	44.873	60.568	0.23	-0.476	0.097	–
He et al.	2023	44.855	60.577	0.189	-0.52	0.093	–

💡 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	5.13	3.05	–	631	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Collinder 34	78.8	44.83	60.57	0.44	-0.35	0.04	-55.55	0.18
SAI 24	30.3	44.83	60.57	0.45	-0.23	0.07	-49.28	0.91

💡 Note: The % column shows the percentage of members that CWNU 4436 shares with each listed object.

Visualization

ℹ️