CWWDL 14262

0.14 UTI

0.33

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.3

C_dup

C3 classification AA

Number of members (P>50%) 33

Radius (P>50% members) 7.5 [arcmin]

C_N 0.33 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.3 Possibly duplicate

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

Overview

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CWWDL 14262 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14262 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	–	89.461	-14.103	1.495	-2.027	1.58	26.549
Chi et al.	2023	89.477	-14.151	1.498	-2.063	1.567	22.247

💡 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
Chi et al.	2023	–	–	–	1	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0367	69.7	89.46	-14.1	1.48	-2.04	1.63	28.57	0.5
CWNU 18	51.5	89.47	-14.09	1.5	-2.01	1.64	26.55	0.11
OC 0366	6.1	89.65	-13.69	1.47	-1.71	1.72	25.66	0.48

💡 Note: The % column shows the percentage of members that CWWDL 14262 shares with each listed object.

Visualization

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