CWNU 2713

0.33 UTI

0.48

C_N

0.04

C_dens

1.0

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 48

Core radius and density 5.6 [pc], 0.2 [pc^-2]

C3 classification AA

C_N 0.48 Poorly populated
C_dens 0.04 Very loose
C_C3 1.0 Very 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

ℹ️

CWNU 2713 is a poorly populated, very loose object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Distant High extinction Massive Metal-rich Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.46 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.46 (50th percentile).

Data

🔍 Search references for CWNU 2713 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	293.395	17.48	0.25	-3.001	-6.295	14.986
Hunt & Reffert	2024	293.399	17.418	0.245	-2.997	-6.299	–
Cavallo et al.	2024	293.384	17.481	0.249	–	–	–
Hunt & Reffert	2023	293.399	17.418	0.245	-2.997	-6.299	–
He et al.	2023	293.421	17.497	0.257	-2.995	-6.298	14.99

💡 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–	4.05	4.67	2.39	28	0.610	1616	–	–
Hunt & Reffert	2024	3.67	4.67	2.39	28	–	1616⁽¹⁾	–	–
Cavallo et al.	2024	4.43	4.42	–	28	0.610	–	–	–
Hunt & Reffert	2023	3.67	4.67	2.39	28	–	–	–	–
He et al.	2023	4.68	5.30	–	2	–	–	–	–

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

Visualization

ℹ️

1 2