CWNU 3077

0.13 UTI

0.66

C_N

0.25

C_dens

0.75

C_C3

0.0

C_lit

0.38

C_dup

N_m (P>50%) 81

Core radius and density 1.9 [pc], 1.2 [pc^-2]

C3 classification AB

C_N 0.66 Moderately populated
C_dens 0.25 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.38 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3077 is a moderately populated, loose object of 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 3077 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	99999–	279.671	-5.398	0.201	-0.772	-2.808	25.574
He et al.	2023	279.669	-5.396	0.215	-0.774	-2.813	25.73

💡 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]	B_frac	BSS
UCC	99999–	4.17	7.25	–	79	–	–	–	–
He et al.	2023	4.17	7.25	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 261	61.7	279.67	-5.4	0.22	-0.78	-2.8	25.57	0.36

💡 Note: The % column shows the percentage of members that CWNU 3077 shares with each listed object.

Visualization

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