CWNU 1058

0.35 UTI

0.69

C_N

0.32

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 88

Stellar density (N₅₀/rad) 1.6 [N/pc²]

C3 classification AB

C_N 0.69 Moderately populated
C_dens 0.32 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1058 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Moderate extinction Very young

Data

🔍 Search references for CWNU 1058 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–	51.401	60.098	0.892	-2.056	-0.733	-9.572
He et al.	2022	51.505	60.111	0.899	-2.052	-0.738	–

💡 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–	–	2.2	–	10	–	–	–	–
He et al.	2022	–	2.20	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1722	36.4	52.68	59.96	0.9	-1.96	-0.7	-18.92	0.29
CWWDL 14458	15.9	52.54	59.8	0.89	-2.01	-0.75	-10.74	0.05
CWNU 1070	13.6	52.68	59.82	0.9	-1.96	-0.75	-27.48	0.29
CWNU 1212	11.4	51.16	59.49	0.9	-2.05	-0.95	-29.94	0.11

💡 Note: The % column shows the percentage of members that CWNU 1058 shares with each listed object.

Visualization

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