CWNU 2927

0.15 UTI

0.78

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.27

C_dup

C3 classification AA

Number of members (P>50%) 175

Radius (P>50% members) 2.1 [arcmin]

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

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

Overview

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CWNU 2927 is a rich, very dense object of very 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 young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction Young

Data

🔍 Search references for CWNU 2927 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	–	258.201	-39.989	0.215	-0.788	-2.291	-35.218
He et al.	2023	258.191	-39.997	0.203	-0.789	-2.275	-35.22

💡 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	3.80	6.20	–	63	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2866	73.1	258.19	-39.99	0.22	-0.81	-2.28	-35.07	0.55

💡 Note: The % column shows the percentage of members that CWNU 2927 shares with each listed object.

Visualization

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