CWWDL 14488

0.08 UTI

0.27

C_N

0.69

C_dens

0.5

C_C3

0.0

C_lit

0.26

C_dup

C3 classification BB

Number of members (P>50%) 27

Radius (P>50% members) 11.2 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.69 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.26 Possibly duplicate

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

Overview

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CWWDL 14488 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a close distance, above 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 14488 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	–	31.557	65.449	1.166	-0.586	-0.422	0.693
Chi et al.	2023	31.503	65.455	1.176	-0.571	-0.378	-4.604

💡 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	–	–	–	50	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 265	74.1	31.92	65.45	1.16	-0.53	-0.44	-4.62	0.45

💡 Note: The % column shows the percentage of members that CWWDL 14488 shares with each listed object.

Visualization

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