CWNU 1244

0.19 UTI

0.57

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.43

C_dup

C3 classification AC

Number of members (P>50%) 65

Radius (P>50% members) 7.8 [arcmin]

C_N 0.57 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.43 Possibly duplicate

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

Overview

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CWNU 1244 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a 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.

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

Moderate extinction Very young

Data

🔍 Search references for CWNU 1244 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	–	326.472	57.589	1.072	-1.419	-3.278	-5.565
He et al.	2022	326.474	57.554	1.047	-1.455	-3.258	–

💡 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	–	2.20	–	7	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0164	56.9	326.51	57.64	1.07	-1.45	-3.26	-5.57	0.4

💡 Note: The % column shows the percentage of members that CWNU 1244 shares with each listed object.

Visualization

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