CWWDL 12297

0.08 UTI

0.31

C_N

0.31

C_dens

0.38

C_C3

0.0

C_lit

0.42

C_dup

C3 classification BC

Number of members (P>50%) 31

Radius (P>50% members) 4.6 [arcmin]

C_N 0.31 Poorly populated
C_dens 0.31 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.42 Possibly duplicate

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

Overview

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CWWDL 12297 is a poorly populated, loose object of low 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 12297 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	–	319.906	55.074	0.301	-3.667	-3.841	–
Chi et al.	2023	319.89	55.088	0.299	-3.647	-3.746	-43.772

💡 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	–	–	–	66	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1601	58.1	319.91	55.07	0.31	-3.69	-3.89	-34.56	0.29

💡 Note: The % column shows the percentage of members that CWWDL 12297 shares with each listed object.

Visualization

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