CWNU 3788

0.40 UTI

0.28

C_N

0.71

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 28

Radius (P>50% members) 0.8 [arcmin]

C_N 0.28 Poorly populated
C_dens 0.71 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 3788 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~12.05 kpc) differs significantly from the median photometric distance (~8.13 kpc).

Very distant Moderate extinction Very young

Data

🔍 Search references for CWNU 3788 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	–	101.404	-7.136	0.083	-0.071	0.82	–
He et al.	2023	101.401	-7.133	0.083	-0.066	0.834	–

💡 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
He et al.	2023	8.13	1.75	–	10	–	–	–	–

Visualization

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