CWWDL 5099

0.09 UTI

0.53

C_N

0.84

C_dens

1.0

C_C3

0.0

C_lit

0.2

C_dup

C3 classification AA

Number of members (P>50%) 56

Radius (P>50% members) 4.8 [arcmin]

C_N 0.53 Moderately populated
C_dens 0.84 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWWDL 5099 is a moderately populated, dense object of very high 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.

⚠️ Warning: This is 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 5099 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	–	157.686	-60.049	0.383	-5.448	2.849	8.985
Chi et al.	2023	157.873	-60.026	0.383	-5.433	2.785	26.811

💡 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	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 259	80.4	157.62	-60.07	0.39	-5.46	2.87	10.47	0.7

💡 Note: The % column shows the percentage of members that CWWDL 5099 shares with each listed object.

Visualization

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