CWWDL 13241

0.21 UTI

0.56

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.44

C_dup

C3 classification AB

Number of members (P>50%) 63

Radius (P>50% members) 4.9 [arcmin]

C_N 0.56 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

ℹ️

CWWDL 13241 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 13241 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	82.247	48.025	0.426	0.609	-1.98	-35.629
Chi et al.	2023	82.254	48.049	0.435	0.629	-1.999	-35.141

💡 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	–	–	–	76	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0276	55.6	82.24	48.02	0.43	0.62	-1.99	-35.98	0.13
UBC 59	39.7	82.24	48.02	0.42	0.62	-1.99	–	0.5

💡 Note: The % column shows the percentage of members that CWWDL 13241 shares with each listed object.

Visualization

ℹ️