CWWDL 13315

0.13 UTI

0.5

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.29

C_dup

C3 classification AB

Number of members (P>50%) 51

Radius (P>50% members) 4.0 [arcmin]

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.29 Possibly duplicate

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

Overview

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CWWDL 13315 is a moderately populated, very 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 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 Young

Data

🔍 Search references for CWWDL 13315 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	–	204.492	-66.659	0.566	-7.555	-2.624	-59.78
Chi et al.	2023	204.496	-66.683	0.568	-7.573	-2.631	-59.78

💡 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	–	–	–	41	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 527	70.6	204.54	-66.65	0.56	-7.54	-2.62	-59.78	0.66

💡 Note: The % column shows the percentage of members that CWWDL 13315 shares with each listed object.

Visualization

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