CWWDL 9197

0.09 UTI

0.0

C_N

0.22

C_dens

0.5

C_C3

0.0

C_lit

0.64

C_dup

C3 classification BB

Number of members (P>50%) 19

Radius (P>50% members) 5.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.22 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

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

Overview

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CWWDL 9197 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, very 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 Very young

Data

🔍 Search references for CWWDL 9197 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	–	165.657	-59.77	0.375	-6.173	1.492	5.205
Chi et al.	2023	165.728	-59.747	0.377	-6.169	1.552	–

💡 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	–	–	–	2	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2487	36.0	165.71	-59.78	0.38	-6.16	1.38	–	0.41

💡 Note: The % column shows the percentage of members that CWWDL 9197 shares with each listed object.

Visualization

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