CWWDL 9706

0.00 UTI

0.51

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 52

Radius (P>50% members) 2.1 [arcmin]

C_N 0.51 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 9706 is a moderately populated, very dense object of very high 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 very likely a duplicate object, which shares a large 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 9706 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	–	270.238	-20.221	0.37	0.199	-0.122	15.491
Chi et al.	2023	270.23	-20.215	0.364	0.176	-0.112	38.273

💡 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	–	–	–	33	-0.040	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UFMG 75	100.0	270.23	-20.22	0.37	0.2	-0.12	20.49	0.61
OC 0016	48.1	270.23	-20.22	0.36	0.19	-0.14	13.84	0.0

💡 Note: The % column shows the percentage of members that CWWDL 9706 shares with each listed object.

Visualization

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