CWNU 4127

0.04 UTI

0.0

C_N

0.15

C_dens

0.62

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AC

Number of members (P>50%) 23

Radius (P>50% members) 20.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.15 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWNU 4127 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate 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.

Close Moderate extinction Young

Data

🔍 Search references for CWNU 4127 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	–	76.556	35.465	1.059	-0.202	-2.97	8.479
He et al.	2023	76.561	35.465	1.065	-0.196	-2.977	18.29

💡 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	0.93	1.85	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1331	76.0	76.71	35.39	1.07	-0.23	-2.99	8.48	0.18

💡 Note: The % column shows the percentage of members that CWNU 4127 shares with each listed object.

Visualization

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