CWNU 3244

0.12 UTI

0.81

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AB

Number of members (P>50%) 249

Radius (P>50% members) 2.4 [arcmin]

C_N 0.81 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWNU 3244 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~4.23 kpc) differs significantly from the median photometric distance (~3.16 kpc).

Distant Very high extinction Young

Data

🔍 Search references for CWNU 3244 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	–	193.859	-63.03	0.236	-6.258	-0.435	-43.752
He et al.	2023	193.86	-63.037	0.241	-6.261	-0.439	-44.16

💡 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.	2023	3.16	5.40	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2539	75.9	193.86	-63.03	0.24	-6.26	-0.43	-43.91	0.51

💡 Note: The % column shows the percentage of members that CWNU 3244 shares with each listed object.

Visualization

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