CWWDL 13697

0.19 UTI

0.34

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.41

C_dup

C3 classification AA

Number of members (P>50%) 34

Radius (P>50% members) 3.6 [arcmin]

C_N 0.34 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.41 Possibly duplicate

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

Overview

ℹ️

CWWDL 13697 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near 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 possibly a duplicate object, which shares a significant 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 13697 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	280.612	-6.907	0.526	-1.03	-2.556	13.019
Chi et al.	2023	280.602	-6.905	0.526	-0.951	-2.572	15.851

💡 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	–	–	–	22	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 102	58.8	280.6	-6.93	0.52	-1.04	-2.54	13.02	0.52

💡 Note: The % column shows the percentage of members that CWWDL 13697 shares with each listed object.

Visualization

ℹ️