CWNU 2415

0.46 UTI

0.63

C_N

0.56

C_dens

1.0

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 76

Core radius and density 1.6 [pc], 2.8 [pc^-2]

C3 classification AA

C_N 0.63 Moderately populated
C_dens 0.56 Moderately dense
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 2415 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Very distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.04 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.04 (50th percentile).

Data

🔍 Search references for CWNU 2415 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	298.379	29.868	0.149	-2.75	-5.275	-5.371
Hunt & Reffert	2024	298.379	29.869	0.142	-2.734	-5.273	-0.965
Cavallo et al.	2024	298.38	29.871	0.143	–	–	–
Hunt & Reffert	2023	298.379	29.869	0.142	-2.734	-5.273	-0.965
He et al.	2023	298.38	29.874	0.173	-2.76	-5.29	-5.37

💡 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–	5.255	3.69	2.77	578	-0.450	2982	–	–
Hunt & Reffert	2024	5.66	3.53	2.77	595	–	2982⁽¹⁾	–	–
Cavallo et al.	2024	4.85	4.45	–	263	-0.450	–	–	–
Hunt & Reffert	2023	5.66	3.53	2.77	596	–	–	–	–
He et al.	2023	4.27	3.85	–	562	–	–	–	–

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

Visualization

ℹ️

1 2