CWNU 1014

0.31 UTI

0.74

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.56

C_dup

C3 classification AA

Number of members (P>50%) 98

Radius (P>50% members) 17.9 [arcmin]

C_N 0.74 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.56 Likely unique

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

Overview

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CWNU 1014 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Low extinction Very young

Data

🔍 Search references for CWNU 1014 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	–	242.201	-39.07	6.276	-9.91	-23.433	-2.536
He et al.	2022	242.153	-39.083	6.299	-9.891	-23.555	–

💡 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.	2022	–	0.35	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 214	85.7	242.2	-39.07	6.28	-9.87	-23.51	-2.45	0.0
OC 0666	43.9	242.17	-39.06	6.31	-10.0	-23.48	-2.45	0.49
CWNU 1004	18.4	240.21	-41.68	6.24	-10.93	-23.51	-2.11	0.41

💡 Note: The % column shows the percentage of members that CWNU 1014 shares with each listed object.

Visualization

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