CWNU 2711

0.03 UTI

0.31

C_N

0.32

C_dens

0.75

C_C3

0.0

C_lit

0.1

C_dup

C3 classification AB

Number of members (P>50%) 31

Radius (P>50% members) 6.4 [arcmin]

C_N 0.31 Poorly populated
C_dens 0.32 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.1 Likely duplicate

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

Overview

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CWNU 2711 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a young 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.

Relatively close Low extinction Young

Data

🔍 Search references for CWNU 2711 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	–	106.041	-6.438	0.426	-1.566	0.619	67.776
He et al.	2023	106.035	-6.418	0.45	-1.567	0.623	–

💡 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	2.09	0.70	–	35	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1149	90.3	106.02	-6.44	0.43	-1.56	0.62	67.78	0.49

💡 Note: The % column shows the percentage of members that CWNU 2711 shares with each listed object.

Visualization

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