CWNU 1268

0.32 UTI

0.0

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.92

C_dup

C3 classification AB

Number of members (P>50%) 21

Radius (P>50% members) 6.1 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.92 Very likely unique

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

Overview

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CWNU 1268 is a sparse, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Moderate extinction Very young

Data

🔍 Search references for CWNU 1268 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	–	250.638	-49.048	0.88	0.422	-4.742	-21.242
He et al.	2022	250.697	-49.053	0.88	0.428	-4.766	–

💡 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	–	2.75	–	8	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1643	100.0	250.31	-48.97	0.84	0.8	-4.53	-28.04	0.2
VVV 083	8.0	250.31	-49.01	0.85	0.84	-4.37	-27.3	0.02
NGC 6193	4.0	250.32	-48.78	0.82	1.28	-4.06	-27.74	0.95

💡 Note: The % column shows the percentage of members that CWNU 1268 shares with each listed object.

Visualization

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