CWWDL 13281

0.05 UTI

0.29

C_N

0.61

C_dens

0.75

C_C3

0.0

C_lit

0.14

C_dup

C3 classification AB

Number of members (P>50%) 29

Radius (P>50% members) 5.7 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.61 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.14 Likely duplicate

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

Overview

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CWWDL 13281 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported 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.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13281 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	–	93.371	1.427	0.537	-0.452	-1.544	37.591
Chi et al.	2023	93.37	1.386	0.533	-0.518	-1.538	37.21

💡 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	–	–	–	35	0.320	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 206	86.2	93.35	1.43	0.53	-0.44	-1.57	34.63	0.51

💡 Note: The % column shows the percentage of members that CWWDL 13281 shares with each listed object.

Visualization

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