CWNU 3872

0.29 UTI

0.73

C_N

0.74

C_dens

0.75

C_C3

0.0

C_lit

0.65

C_dup

C3 classification AB

Number of members (P>50%) 96

Radius (P>50% members) 5.2 [arcmin]

C_N 0.73 Moderately populated
C_dens 0.74 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.65 Likely unique

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

Overview

ℹ️

CWNU 3872 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction Very young

Data

🔍 Search references for CWNU 3872 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	209.907	-61.379	0.297	-5.202	-1.89	-24.553
He et al.	2023	209.886	-61.379	0.29	-5.212	-1.866	–

💡 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	3.09	5.50	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
MCM 41	35.4	209.87	-61.38	0.31	-5.37	-1.88	-26.16	0.43
HSC 2627	26.0	209.89	-61.38	0.29	-5.19	-1.88	–	0.14

💡 Note: The % column shows the percentage of members that CWNU 3872 shares with each listed object.

Visualization

ℹ️