CWWDL 13308

0.07 UTI

0.57

C_N

0.58

C_dens

0.75

C_C3

0.0

C_lit

0.17

C_dup

C3 classification AB

Number of members (P>50%) 64

Radius (P>50% members) 8.4 [arcmin]

C_N 0.57 Moderately populated
C_dens 0.58 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

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

Overview

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CWWDL 13308 is a moderately 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, very 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 Very young

Data

🔍 Search references for CWWDL 13308 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	–	136.922	-52.924	0.521	-6.024	4.306	10.757
Chi et al.	2023	136.833	-52.873	0.521	-5.955	4.324	10.228

💡 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	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 249	82.8	136.95	-52.95	0.52	-6.05	4.28	9.84	0.65

💡 Note: The % column shows the percentage of members that CWWDL 13308 shares with each listed object.

Visualization

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