CWWDL 13505

0.03 UTI

0.0

C_N

0.06

C_dens

0.38

C_C3

0.0

C_lit

0.36

C_dup

C3 classification BC

Number of members (P>50%) 16

Radius (P>50% members) 9.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.36 Possibly duplicate

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

Overview

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CWWDL 13505 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age 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 Intermediate age

Data

🔍 Search references for CWWDL 13505 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	–	12.117	61.168	0.397	-2.826	-0.823	–
Chi et al.	2023	12.143	61.256	0.45	-2.807	-0.835	–

💡 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	–	–	–	457	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1207	64.0	12.08	61.17	0.37	-2.86	-0.82	–	0.36

💡 Note: The % column shows the percentage of members that CWWDL 13505 shares with each listed object.

Visualization

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