CWWDL 14261

0.01 UTI

0.3

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AB

Number of members (P>50%) 30

Radius (P>50% members) 5.9 [arcmin]

C_N 0.3 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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CWWDL 14261 is a poorly populated, very dense object of 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 very likely a duplicate object, which shares a large 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 14261 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	–	90.894	-9.754	1.165	-2.052	1.623	44.56
Chi et al.	2023	90.945	-9.804	1.143	-2.009	1.589	41.407

💡 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	–	–	–	3	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0362	96.7	90.89	-9.79	1.19	-2.11	1.64	39.52	0.47
Theia 15	53.3	90.87	-9.75	1.18	-2.24	1.62	46.29	0.02
OC 0361	30.0	90.56	-9.92	1.23	-2.02	1.77	18.13	0.35

💡 Note: The % column shows the percentage of members that CWWDL 14261 shares with each listed object.

Visualization

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