CWNU 2704

0.04 UTI

0.39

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.13

C_dup

C3 classification DB

Number of members (P>50%) 39

Radius (P>50% members) 1.9 [arcmin]

C_N 0.39 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.13 Likely duplicate

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

Overview

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CWNU 2704 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a very 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.

Distant Low extinction Very young

Data

🔍 Search references for CWNU 2704 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	–	185.053	-62.861	0.286	-6.435	-0.109	–
He et al.	2023	185.056	-62.862	0.289	-6.439	-0.116	–

💡 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	3.02	0.50	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
VVV 012	87.2	185.05	-62.86	0.29	-6.43	-0.11	–	0.36
CWWDL 1492	71.8	185.04	-62.86	0.28	-6.47	-0.11	–	0.0

💡 Note: The % column shows the percentage of members that CWNU 2704 shares with each listed object.

Visualization

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