CWNU 195

0.40 UTI

0.25

C_N

0.4

C_dens

0.75

C_C3

0.31

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 25

Radius (P>50% members) 6.3 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.4 Loose
C_C3 0.75 High quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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CWNU 195 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 195 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	–	82.967	29.081	0.515	0.384	-2.481	–
Zhang et al.	2024	82.971	29.071	–	–	–	–
Hunt & Reffert	2024	82.971	29.071	0.507	0.426	-2.475	–
Cavallo et al.	2024	82.998	29.084	0.51	–	–	–
Hunt & Reffert	2023	82.971	29.071	0.507	0.426	-2.475	–
He et al.	2022	82.992	29.081	0.48	0.52	-2.5	–

💡 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
Zhang et al.	2024	–	–	–	–	-0.181*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	282*	–	–
Cavallo et al.	2024	1.86	1.43	–	126	0.430	–	–	–
Hunt & Reffert	2023	1.85	1.88	1.83	72	–	–	–	–
He et al.	2022	1.82	2.04	–	32	-0.419	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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