Alessi 11

(MWSC 3321)

0.03 UTI

0.0

C_N

0.04

C_dens

0.12

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 12

Stellar density (N₅₀/rad) 0.2 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Alessi 11 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, well below the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Dias et al. (2002)
Asterism (Alessi, B. S. 2005, private communication); cat V3.5 (Jan 2016)

Data

🔍 Search references for Alessi 11 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–	305.3	18.376	0.273	-3.319	-5.319	-39.681
Bica et al.	2019	305.348	18.357	–	–	–	–
Alessi et al.	2003	305.3	18.4	–	-0.3	-9.6	–

💡 Note: The UCC values are estimated from its identified members.

Visualization

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