CWNU 242

0.10 UTI

0.56

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AC

Number of members (P>50%) 63

Radius (P>50% members) 3.1 [arcmin]

C_N 0.56 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate 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 242 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied 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.

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 242 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	–	129.99	-48.231	0.454	-4.991	5.067	23.009
He et al.	2022	130.01	-48.243	0.46	-5.02	5.07	–

💡 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	1.70	1.44	–	63	-0.419	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 168	77.8	129.99	-48.23	0.46	-4.98	5.08	23.01	0.0
UBC 1450	76.2	129.99	-48.23	0.46	-4.99	5.09	35.4	0.55

💡 Note: The % column shows the percentage of members that CWNU 242 shares with each listed object.

Visualization

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