CWWDL 772

0.13 UTI

0.58

C_N

0.34

C_dens

0.12

C_C3

0.0

C_lit

0.63

C_dup

C3 classification DC

Number of members (P>50%) 67

Radius (P>50% members) 6.4 [arcmin]

C_N 0.58 Moderately populated
C_dens 0.34 Loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.63 Likely unique

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

Overview

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CWWDL 772 is a moderately populated, loose object of very low C3 quality. Its parallax locates it at a moderate distance, below 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. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 772 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	–	154.024	-59.042	0.296	-7.005	3.773	13.865
Chi et al.	2023	154.012	-59.056	0.291	-7.026	3.762	5.543

💡 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	–	–	–	41	-0.040	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 782	37.3	153.98	-59.03	0.28	-7.2	3.93	8.24	0.51
HSC 2330	20.9	153.98	-59.03	0.28	-7.28	3.95	8.24	0.21

💡 Note: The % column shows the percentage of members that CWWDL 772 shares with each listed object.

Visualization

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