CWNU 3072

0.03 UTI

0.55

C_N

0.46

C_dens

0.25

C_C3

0.0

C_lit

0.13

C_dup

C3 classification DB

Number of members (P>50%) 60

Radius (P>50% members) 2.8 [arcmin]

C_N 0.55 Moderately populated
C_dens 0.46 Loose
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 3072 is a moderately populated, loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by high 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.

(*): The parallax distance estimate (~6.24 kpc) differs significantly from the median photometric distance (~10.47 kpc).

Extremely distant High extinction Very young

Data

🔍 Search references for CWNU 3072 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	–	332.615	57.737	0.16	-2.861	-2.017	–
He et al.	2023	332.606	57.746	0.161	-2.864	-2.019	–

💡 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	10.47	4.45	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 796	86.7	332.63	57.74	0.16	-2.86	-2.02	-58.94	0.05
FSR 0354	76.7	332.75	57.69	0.17	-2.89	-2.03	-48.45	0.45
LP 24	8.3	332.61	57.86	0.2	-2.85	-1.79	–	0.14

💡 Note: The % column shows the percentage of members that CWNU 3072 shares with each listed object.

Visualization

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