CWWDL 13478

0.18 UTI

0.0

C_N

0.3

C_dens

1.0

C_C3

0.0

C_lit

0.68

C_dup

C3 classification AA

Number of members (P>50%) 24

Radius (P>50% members) 6.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.3 Loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.68 Likely unique

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

Overview

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CWWDL 13478 is a sparse, loose object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate 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 13478 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	–	276.791	-14.977	0.473	-0.692	-2.772	–
Chi et al.	2023	276.791	-14.962	0.461	-0.708	-2.775	-24.497

💡 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	–	–	–	2	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1014	32.0	276.57	-15.14	0.48	-0.72	-2.73	–	0.31

💡 Note: The % column shows the percentage of members that CWWDL 13478 shares with each listed object.

Visualization

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