CWWDL 14698

0.43 UTI

0.74

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.79

C_dup

C3 classification AA

Number of members (P>50%) 97

Radius (P>50% members) 46.5 [arcmin]

C_N 0.74 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.79 Very likely unique

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

Overview

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CWWDL 14698 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above 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 very likely a unique object, which shares a small 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 14698 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	–	244.651	-25.038	6.282	-10.791	-21.611	-4.485
Chi et al.	2023	244.418	-24.785	6.293	-10.795	-21.542	-7.962

💡 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	–	–	–	1	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2907	100.0	244.86	-24.99	6.37	-10.63	-21.5	-5.44	0.41
OCSN 246	20.6	245.41	-24.73	6.71	-10.64	-22.4	-3.67	0.45

💡 Note: The % column shows the percentage of members that CWWDL 14698 shares with each listed object.

Visualization

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