CWNU 2414

0.39 UTI

0.38

C_N

0.46

C_dens

1.0

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 38

Core radius and density 1.6 [pc], 2.3 [pc^-2]

C3 classification AA

C_N 0.38 Poorly populated
C_dens 0.46 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 2414 is a poorly populated, 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 near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Distant High extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.56 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.56 (50th percentile).

Data

🔍 Search references for CWNU 2414 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	299.05	26.068	0.293	-3.131	-5.724	10.646
Hunt & Reffert	2024	299.047	26.069	0.297	-3.135	-5.708	24.715
Cavallo et al.	2024	299.1	26.087	0.297	–	–	–
Hunt & Reffert	2023	299.047	26.069	0.297	-3.135	-5.708	24.715
He et al.	2023	299.071	26.08	0.295	-3.127	-5.716	–

💡 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–	3.24	4.365	2.46	11	0.300	903	–	–
Hunt & Reffert	2024	3.16	4.32	2.46	11	–	903⁽¹⁾	–	–
Cavallo et al.	2024	3.53	4.41	–	11	0.300	–	–	–
Hunt & Reffert	2023	3.17	4.32	2.46	11	–	–	–	–
He et al.	2023	3.31	5.05	–	16	–	–	–	–

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

Visualization

ℹ️

1 2