Alessi 145

(UBC 13)

0.50 UTI

0.73

C_N

0.2

C_dens

0.75

C_C3

0.4

C_lit

1.0

C_dup

N₅₀ (P>50% members) 96

Stellar density (N₅₀/rad) 1.0 [N/pc²]

C3 classification AB

C_N 0.73 Moderately populated
C_dens 0.2 Very loose
C_C3 0.75 High quality
C_lit 0.4 Poorly studied
C_dup 1.0 Unique

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

Overview

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Alessi 145 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Close Low extinction Near-solar metallicity Intermediate age

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for Alessi 145 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–	120.85	3.465	1.6	-7.854	-1.245	25.043
Alfonso et al.	2024	120.696	3.693	1.587	-7.801	-1.39	–
Zhang et al.	2024	120.954	3.985	–	–	–	–
Tarricq et al.	2022	120.761	2.697	1.583	-7.68	-1.199	–
Cantat-Gaudin et al.	2020	120.914	3.54	1.609	-7.749	-1.13	–
Cantat-Gaudin & Anders	2020	120.914	3.54	1.609	-7.749	-1.13	–
Bica et al.	2019	120.894	3.611	–	–	–	–
Castro-Ginard et al.	2018	120.897	3.61	1.607	-7.768	-1.163	22.91

💡 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–	0.625	0.0	–	182	-0.064	–	–	–
Alfonso et al.	2024	0.63	0.00	–	45	-0.066	–	–	–
Zhang et al.	2024	–	–	–	–	-0.062⁽¹⁾	–	–	–
Tarricq et al.	2022	0.62	–	–	191	–	–	–	–
Cantat-Gaudin et al.	2020	0.63	0.00	–	182	–	–	–	–
Cantat-Gaudin & Anders	2020	0.61	–	–	–	–	–	–	–

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

Visualization

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