CWNU 1337

0.18 UTI

0.52

C_N

0.58

C_dens

0.62

C_C3

0.0

C_lit

0.51

C_dup

C3 classification AC

Number of members (P>50%) 53

Radius (P>50% members) 10.5 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.58 Moderately dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.51 Likely unique

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

Overview

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CWNU 1337 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Moderate extinction Very young

Data

🔍 Search references for CWNU 1337 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	–	111.029	-24.397	0.717	-2.141	2.233	31.616
He et al.	2023	111.015	-24.416	0.744	-2.128	2.201	–

💡 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	1.29	1.35	–	8	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Majaess 90	49.1	111.19	-24.48	0.74	-2.16	2.27	31.62	0.52
Ivanov 6	5.7	111.06	-24.64	0.72	-2.05	2.69	18.64	0.67

💡 Note: The % column shows the percentage of members that CWNU 1337 shares with each listed object.

Visualization

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