CWNU 1700

0.03 UTI

0.0

C_N

0.4

C_dens

0.38

C_C3

0.0

C_lit

0.2

C_dup

N₅₀ (P>50% members) 20

Stellar density (N₅₀/rad) 2.0 [N/pc²]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.4 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CWNU 1700 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by very high extinction. It is catalogued as a 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.

Distant Very high extinction Very young

Data

🔍 Search references for CWNU 1700 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	291.732	13.952	0.276	-3.071	-5.889	59.282
He et al.	2023	291.73	13.953	0.285	-3.074	-5.884	–

💡 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–	4.17	5.85	–	2	–	–	–	–
He et al.	2023	4.17	5.85	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0129	80.0	291.73	13.95	0.28	-3.06	-5.88	59.28	0.35

💡 Note: The % column shows the percentage of members that CWNU 1700 shares with each listed object.

Visualization

ℹ️