CWNU 1476

0.41 UTI

0.44

C_N

0.59

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 44

Stellar density (N₅₀/rad) 2.9 [N/pc²]

C3 classification AA

C_N 0.44 Poorly populated
C_dens 0.59 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

CWNU 1476 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 1476 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	270.792	-23.692	0.331	-0.077	-1.036	36.664
He et al.	2023	270.768	-23.715	0.342	-0.078	-1.031	–

💡 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]	B_frac	BSS
UCC	99999–	2.69	3.9	–	11	–	–	–	–
He et al.	2023	2.69	3.90	–	11	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1647	65.9	270.79	-23.68	0.33	-0.08	-1.03	–	0.0

💡 Note: The % column shows the percentage of members that CWNU 1476 shares with each listed object.

Visualization

ℹ️