CWNU 1070

0.29 UTI

0.33

C_N

0.36

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 33

Radius (P>50% members) 13.3 [arcmin]

C_N 0.33 Poorly populated
C_dens 0.36 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

ℹ️

CWNU 1070 is a poorly 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 moderate 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 1070 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	52.677	59.818	0.898	-1.958	-0.747	-27.482
He et al.	2022	52.658	59.843	0.902	-1.939	-0.734	–

💡 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	–	1.85	–	14	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1722	100.0	52.68	59.96	0.9	-1.96	-0.7	-18.92	0.29
CWWDL 14458	57.6	52.54	59.8	0.89	-2.01	-0.75	-10.74	0.05
CWNU 1058	36.4	51.4	60.1	0.89	-2.06	-0.73	-9.57	0.35

💡 Note: The % column shows the percentage of members that CWNU 1070 shares with each listed object.

Visualization

ℹ️