CWNU 1410

0.34 UTI

0.36

C_N

0.34

C_dens

0.5

C_C3

0.25

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 36

Radius (P>50% members) 7.0 [arcmin]

C_N 0.36 Poorly populated
C_dens 0.34 Loose
C_C3 0.5 Intermediate quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

CWNU 1410 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported 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.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1410 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	105.975	-4.024	0.442	-0.735	0.332	–
Hunt & Reffert	2024	105.954	-4.016	0.442	-0.735	0.321	–
Cavallo et al.	2024	105.94	-4.001	0.439	–	–	–
Hunt & Reffert	2023	105.954	-4.016	0.442	-0.735	0.321	–
He et al.	2023	105.976	-4.002	0.454	-0.731	0.332	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	91*	–	–
Cavallo et al.	2024	1.81	0.40	–	398	0.030	–	–	–
Hunt & Reffert	2023	2.03	0.55	0.63	134	–	–	–	–
He et al.	2023	2.09	0.80	–	35	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1771	25.0	105.66	-3.81	0.49	-0.67	0.32	–	0.12

💡 Note: The % column shows the percentage of members that CWNU 1410 shares with each listed object.

Visualization

ℹ️

1 2