CWNU 361

0.47 UTI

0.28

C_N

0.95

C_dens

0.38

C_C3

0.38

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 28

Radius (P>50% members) 8.5 [arcmin]

C_N 0.28 Poorly populated
C_dens 0.95 Very dense
C_C3 0.38 Low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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CWNU 361 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 361 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	–	64.336	42.82	1.017	2.116	-1.368	-26.128
Zhang et al.	2024	64.354	42.809	–	–	–	–
Hunt & Reffert	2024	64.354	42.809	1.024	2.09	-1.369	-27.104
Cavallo et al.	2024	64.332	42.828	1.019	–	–	–
Hunt & Reffert	2023	64.354	42.809	1.024	2.09	-1.369	-27.104
He et al.	2022	64.367	42.794	1.022	2.095	-1.36	–
He et al.	2022	64.354	42.804	0.98	2.12	-1.37	–

💡 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
Zhang et al.	2024	–	–	–	–	-0.020*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	115*	–	–
Cavallo et al.	2024	1.07	1.92	–	34	0.100	–	–	–
Hunt & Reffert	2023	0.95	1.60	0.89	125	–	–	–	–
He et al.	2022	–	2.10	–	32	–	–	–	–
He et al.	2022	0.98	2.10	–	32	-0.930	–	–	–

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

Visualization

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