CWWDL 10273

0.06 UTI

0.0

C_N

0.28

C_dens

0.12

C_C3

0.0

C_lit

0.72

C_dup

C3 classification DC

Number of members (P>50%) 24

Radius (P>50% members) 6.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.28 Loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.72 Likely unique

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

Overview

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CWWDL 10273 is a sparse, loose object of very 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.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 10273 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	–	302.87	36.503	0.429	-2.51	-5.609	–
Chi et al.	2023	302.893	36.474	0.437	-2.449	-5.538	13.665

💡 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	–	–	–	29	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 368	28.0	302.86	36.51	0.44	-2.57	-5.78	-42.81	0.54
CWWDL 10272	12.0	302.89	36.57	0.42	-2.78	-5.7	-2.17	0.05
CWWDL 13929	4.0	302.83	36.51	0.45	-2.62	-5.79	-28.41	0.09

💡 Note: The % column shows the percentage of members that CWWDL 10273 shares with each listed object.

Visualization

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