CWNU 1715

0.41 UTI

0.33

C_N

0.84

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 33

Core radius and density 0.8 [pc], 4.2 [pc^-2]

C3 classification BA

C_N 0.33 Poorly populated
C_dens 0.84 Dense
C_C3 0.75 High quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1715 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.14 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.14 (50th percentile).

Data

🔍 Search references for CWNU 1715 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–	50.933	67.348	0.205	0.135	-0.223	-46.71
Hunt & Reffert	2024	50.936	67.348	0.186	0.102	-0.194	-46.705
Cavallo et al.	2024	50.964	67.344	0.189	–	–	–
Hunt & Reffert	2023	50.936	67.348	0.186	0.102	-0.194	-46.705
He et al.	2023	50.936	67.349	0.22	0.138	-0.218	–

💡 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–	4.78	2.95	1.72	468	-0.020	839	–	–
Hunt & Reffert	2024	4.55	2.70	1.72	490	–	839⁽¹⁾	–	–
Cavallo et al.	2024	5.32	3.28	–	234	-0.020	–	–	–
Hunt & Reffert	2023	4.55	2.70	1.72	490	–	–	–	–
He et al.	2023	5.01	3.20	–	447	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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