CWNU 3979

0.31 UTI

0.28

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 28

Radius (P>50% members) 1.2 [arcmin]

C_N 0.28 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

ℹ️

CWNU 3979 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a large^* distance, above 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.

(*): The parallax distance estimate (~5.22 kpc) differs significantly from the median photometric distance (~8.71 kpc).

Very distant Very high extinction Very young

Data

🔍 Search references for CWNU 3979 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	289.032	15.114	0.192	-2.43	-4.954	58.278
He et al.	2023	289.033	15.11	0.192	-2.421	-4.95	58.28

💡 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	8.71	5.35	–	2	–	–	–	–

Visualization

ℹ️