CWNU 373

0.26 UTI

0.28

C_N

0.42

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 28

Radius (P>50% members) 9.5 [arcmin]

C_N 0.28 Poorly populated
C_dens 0.42 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 373 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~1.32 kpc) differs significantly from the median photometric distance (~1.00 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Very metal-poor Intermediate age

Data

🔍 Search references for CWNU 373 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	–	294.911	23.665	0.756	-0.579	-3.628	-20.229
He et al.	2022	294.934	23.637	0.75	-0.56	-3.66	–

💡 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	1.00	2.10	–	501	-1.335	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2921	78.6	294.86	23.73	0.76	-0.59	-3.63	-20.23	0.03

💡 Note: The % column shows the percentage of members that CWNU 373 shares with each listed object.

Visualization

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