CWWDL 2458

0.08 UTI

0.4

C_N

0.63

C_dens

0.5

C_C3

0.0

C_lit

0.28

C_dup

C3 classification BB

Number of members (P>50%) 40

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

C_N 0.4 Poorly populated
C_dens 0.63 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

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CWWDL 2458 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate 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 2458 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	–	299.85	31.174	0.326	-2.44	-5.222	14.813
Chi et al.	2023	299.889	31.18	0.33	-2.5	-5.18	-13.113

💡 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	–	–	–	27	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1078	72.5	299.85	31.18	0.33	-2.39	-5.25	-2.79	0.56

💡 Note: The % column shows the percentage of members that CWWDL 2458 shares with each listed object.

Visualization

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