CWNU 510

0.22 UTI

0.26

C_N

0.7

C_dens

0.75

C_C3

0.0

C_lit

0.65

C_dup

C3 classification BA

Number of members (P>50%) 26

Radius (P>50% members) 26.6 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.7 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.65 Likely unique

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

Overview

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CWNU 510 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

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

Very close Low extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 510 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	–	287.666	39.517	2.843	1.832	-1.721	-19.985
He et al.	2022	287.823	39.581	2.84	1.81	-1.72	-18.1

💡 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
He et al.	2022	0.41	0.36	–	40	0.457	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 101	34.6	284.76	39.8	2.84	1.39	-1.74	-19.17	0.53
OCSN 106	11.5	284.94	39.87	2.8	1.61	-1.65	-21.64	0.0

💡 Note: The % column shows the percentage of members that CWNU 510 shares with each listed object.

Visualization

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