CWNU 1208

0.06 UTI

0.0

C_N

0.36

C_dens

0.25

C_C3

0.0

C_lit

0.52

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 1.8 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.36 Loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1208 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Moderate extinction Very young

Data

🔍 Search references for CWNU 1208 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	99.069	9.949	0.842	-1.577	-0.87	16.049
He et al.	2022	99.097	9.973	0.842	-1.573	-0.894	–

💡 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–	–	1.25	–	14	–	–	–	–
He et al.	2022	–	1.25	–	14	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1797	76.0	99.07	9.93	0.84	-1.58	-0.91	16.05	0.09
CWNU 81	48.0	98.96	10.24	0.85	-1.61	-0.88	5.04	0.11

💡 Note: The % column shows the percentage of members that CWNU 1208 shares with each listed object.

Visualization

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