CWWDL 14650

0.07 UTI

0.26

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.15

C_dup

C3 classification AA

Number of members (P>50%) 26

Radius (P>50% members) 10.4 [arcmin]

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

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

Overview

ℹ️

CWWDL 14650 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a 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.

⚠️ 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 Very young

Data

🔍 Search references for CWWDL 14650 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	315.17	52.303	1.776	1.202	-3.509	-27.653
Chi et al.	2023	315.181	52.321	1.786	1.15	-3.47	-33.497

💡 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	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 144	84.6	315.15	52.3	1.78	1.25	-3.53	-25.22	0.58

💡 Note: The % column shows the percentage of members that CWWDL 14650 shares with each listed object.

Visualization

ℹ️