CWWDL 2852

0.08 UTI

0.0

C_N

0.16

C_dens

0.62

C_C3

0.0

C_lit

0.48

C_dup

C3 classification AC

Number of members (P>50%) 18

Radius (P>50% members) 4.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.48 Possibly duplicate

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

Overview

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CWWDL 2852 is a sparse, very loose 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 2852 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	–	301.627	36.356	0.267	-2.934	-5.984	19.58
Chi et al.	2023	301.603	36.362	0.251	-2.911	-5.901	10.084

💡 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	–	–	–	76	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1092	52.0	301.63	36.36	0.28	-2.98	-6.14	-16.38	0.46

💡 Note: The % column shows the percentage of members that CWWDL 2852 shares with each listed object.

Visualization

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