CWNU 2979

0.44 UTI

0.7

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 90

Radius (P>50% members) 1.4 [arcmin]

C_N 0.7 Moderately populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 2979 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate^* 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 (~4.54 kpc) differs significantly from the median photometric distance (~8.13 kpc).

Very distant Very high extinction Very young

Data

🔍 Search references for CWNU 2979 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	8.294	65.12	0.22	-2.512	-0.353	-86.839
He et al.	2023	8.292	65.119	0.191	-2.51	-0.341	-86.84

💡 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	8.13	5.20	–	5	–	–	–	–

Visualization

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